METHOD FOR REBINNING AND FOR CORRECTING CONE BEAM ERROR IN A FAN BEAM COMPUTED TOMOGRAPHIC SCANNER SYSTEM

Abstract: A method of reconstructing data acquired on a fan beam ct system firstly rebins the data to parallel beam format using limited angle weighting fold-over redundant data by adding corner rays of one scan to the center rays of another scan. (52A) denotes column interpolation for the first scan data and (52b) denotes column interpolation for the second scan data. After the two scans are weighted, the sinogram corner of one scan is added to the sinogram corner of the other scan. By so doing, fold-over (56) is obtained. Further interpolation is avoided after the first one-dimensional interpolation. The resultant sinogram undergoes a final rebinning step (60) that results in a row transformation.

Description: METHOD FOR REBINNING AND FOR CORRECTING CONE BEAM ERROR IN A FAN BEAM COMPUTED TOMOGRAPHIC SCANNER SYSTEM FIELD OF THE INVENTION The present invention relates generally to computed tomography X-ray systems, and more particularly to a method for rebinning fan beam data, and for correcting cone beam error in a fan beam computed tomographic scanner system using a parallel beam reconstruction algorithm. BACKGROUND OF THE INVENTION Early in this century, the Austrian mathematician J. Radon demonstrated that a two-dimensional slice of a three- dimensional object may be reproduced from the set of all of its projections. Computed tomography ("CT") X-ray systems generate a set of X-ray beam projections through an object to be examined. The resultant detected X-ray data are computer processed to reconstruct a tomographic image-slice of the object. CT systems subject the object under examination to one or more pencil-like X-ray beams from all possible directions. The X-ray data may be generated in fan beam format (as is the case for the present invention) , or in parallel beam format. In a fan beam system, the X-rays radiate from a source and are collected in a fan. By contrast, in a parallel beam system the X-rays are all parallel within a view. In either system, a view is one projection of the object onto the detectors, and a scan is a collection of all of the views . In a fan beam scanning electron beam system such as described in U. S. Patent no. 4,521,900 to Rand, or U.S. Patent no. 4,352,021 to Boyd, an electron beam is produced by an electron gun and is accelerated downstream along the z-axis of an evacuated chamber. Further downstream a beam optical system deflects the electron beam into a scanning path, typically about 210°. The deflected beam is then focussed upon a suitable target, typically a large arc of tungsten material, which produces a fan beam of X-rays. The emitted X-rays penetrate an object (e.g., a patient) that is disposed along the z-axis and lying within a so- called reconstruction circle. X-ray beams passing through the object are attenuated by various amounts, depending upon the nature of the object traversed (e.g., bone, tissue, metal) . One or more X-ray detectors, disposed on the far side of the object, receive these beams and provide signals proportional to the strength of the incoming X-rays. Typically the output data from the detectors are processed using a filtered backprojection algorithm. Detector data representing the object scanned from many directions are arranged to produce image profiles for each scan direction. Since the X-rayed object is not homogeneous, these profiles will vary in intensity with the amount of radiation detected by the various detectors on the various scans. The rays from the various projections are then superimposed, or backprojected, to produce a computed tomographic image of the original object. The thus processed data are used to produce a reconstructed image of a slice of the object, which image may be displayed on a video monitor. Systems similar to what is described in the above patents to Rand or Boyd are manufactured by Imatron, Inc., located in South San Francisco, California. These systems are termed "short scan" because the views used for reconstructing an object image cover 180° plus the fan beam angle (about 30°) , e.g., about 210° total, rather than a full 360°. In these systems, the X-ray detectors also span 180° plus the fan angle, and define a first plane that is orthogonal to the z-axis. The source of the X-rays scans or travels within a second plane, also orthogonal to the z-axis, but not necessarily coincident with the first plane. However in scanning electron beam fourth-generation CT systems, the large evacuated chamber and distance separating the target and detectors, can result in these two planes being offset by a dimension Δz, that may be in the range of a cm or so. Thus, while ideally reconstruction creates an image in a plane perpendicular to the z-axis using views acquired within that plane, due to the cone angle, each acquired view is not perpendicular to the z-axis. This Δz offset causes the X-ray beam to somewhat misalign and sweep out a shallow cone during a scan, and unless the cone beam geometry is accounted for during reconstruction, cone beam error results. Unless corrected, cone beam error produces a reconstructed image that includes unwanted cone beam artifacts that appear as streaks in the reconstructed, displayed image. To display a reconstructed image of the object slice requires computer intensive reconstruction techniques. Computed tomography is the method of determining the cross section of an X-rayed object by using projections of the object from many different angles. A mathematical reconstruction algorithm is used to reconstruct the object's cross section from the fan beam projections, represented by the detected data. Computed tomography reconstruction algorithms exist for fan beam data and for parallel beam data. Such fan beam algorithms are described, for example, in "Principles of Computerized Tomographic Imaging" by Avinash Kak and Malcolm Slaney, IEEE Press, N.Y. (1987) . The reference "Optimal Short-Scan Convolution Reconstruction for Fan Beam CT", by Dennis Parker, Med. Phys. , 9:254-257 (1982) , describes weights used in short scan fan beam algorithms. In general, attempting to process fan beam data in real time, e.g., a few seconds or less, requires using custom designed computer equipment . This results because fan beam reconstruction techniques involve spatial domain backprojection algorithms, which are extremely computer intensive in that many computational operations are required. Thus, generally, fan beam reconstruction is less desirable than parallel beam reconstruction. By contrast, there exist parallel beam reconstruction techniques that use transform domain algorithms that execute rapidly using conventional computer array processors. Relying upon customized backprojection equipment is not desirable because a modification of the CT system can require modification of the backprojection equipment, a costly and time consuming process. Further, relatively few companies produce custom designed backprojectors, and from an engineering and business standpoint, it is undesirable for the CT system manufacturer to rely on sole-source equipment such as backprojectors. It is therefore preferred that parallel beam reconstruction techniques be practiced, for reasons of speed and for ease of implementation using commercially available array processors. Among parallel beam reconstruction techniques are the so-called gridding Fourier inversion algorithms, wherein each view is transformed, convolved with a gridding function, and then added into a two-dimensional Fourier transform of the image. If such method is done for but one view, the resulting image equals the backprojection of that view, using a filtered backprojection algorithm. See, for example, J.D. O'Sullivan, "A Fast Sine Function Gridding Algorithm for Fourier Inversion in Computer Tomography", IEEE Trans on Medical Imaging, vol. MI-4, no. 4, pp 200-207, December, 1985, and J. Jackson, C. Meyer, D. Nishimura, A. Macovski, "Selection of a Convolution Function for Fourier Inversion Using Gridding", IEEE Trans on Medical Imaging, vol. MI-10, no. 3, pp 473-478. 7Another parallel beam algorithm was disclosed in M. Tabei, M. Ueda, "Backprojection by Unsampled Fourier Series Expansion and Interpolated FFT" , IEEE Trans on Image Proc. , vol. 1, No. 1, pp 77-87, a gridding technique, where a Gaussian gridding function was used, as such functions may be calculated rapidly on the fly. While Tabei-type parallel beam reconstruction algorithms have many advantages, they cannot be used with fan beam data. Fortunately, however, so-called rebinning techniques are known for transforming or converting fan beam data to parallel beam data, whereupon fast parallel beam algorithms such as that disclosed by Tabei may be used for reconstruction. One such rebinning algorithm is described by Gabor Herman, in Image Reconstructions from Projections, 1980 Academic Press, N.Y. However, even if fan beam data are suitably rebinned for reconstruction using a fast parallel beam reconstruction algorithm, the Δz offset noted above produces a so-called cone beam artifact in the reconstructed image. Further, conventional short scan fan beam to parallel beam rebinning techniques discard redundant data appearing at the top and bottom of the fan beam sinogram. This practice is undesirable because, in medical applications, the redundant regions of the sinogram represent data for which the patient was irradiated. Further, discarding the redundant data reduces the signal to noise ratio. What is needed is a method of retaining redundant data in a fan beam sinogram during a rebinning operation. Preferably such modified rebinning method would make the resultant parallel beam data suitable for correcting cone beam error. Further, there is a need for a modified Tabei-type algorithm capable of correcting for cone beam error, and capable of permitting imaging zooming on the displayed image from a point other than the center of the image. What is needed is a reconstruction method that permits a zoom view of the reconstructed image, from any point on the image. The present invention describes such a modified rebinning procedure, and a modified Tabei-type parallel beam reconstruction procedure, whereby cone beam error is substantially reduced. Further, the present invention provides non-center zooming of the reconstructed displayed image. Further, the present invention may be implemented with conventional array processors, and is faster executing than the Tabei reconstruction method. SUMMARY OF THE INVENTION The present invention uses spatial techniques and transform techniques to correct for cone beam error in a fan beam CT system. Two or more CT scans, each separated by a small distance in the z-direction, are used to produce one reconstructed image with substantially reduced cone beam errors. A rebinning step is used to transform the fan beam views into parallel beam format, which format permits rapid reconstruction using a modified parallel beam reconstruction algorithm. A special folding step is incorporated into the rebinning step that makes use of redundant rays. Once rebinned, the views are reconstructed using a gridding- type Fourier technique that has been modified according to the present invention. The views of each scan are treated in such a way as to effect a weighting of the backprojected view by a function that depends on the distance from the reconstruction circle edge, measured in the direction of the view. Rather than perform the weighting in the spatial domain using a custom backprojector, the present invention performs the weighting in the Fourier domain, by convolving the transformed view with the Fourier transform of a suitable weighting function. Reconstruction according to the present invention is carried out using general purpose array processors, and there is no speed penalty for high order interpolation during backprojection. The quality of the reconstructed image is excellent, and zoomed, off-axis reconstructions are possible. Thus, in a first aspect, the present invention provides a method for rebinning fan beam data into parallel beam format, a step necessary to make use of a fast executing parallel beam reconstruction algorithm. Applicant's rebinning method consists of two one-dimensional interpolation steps with a folding step in between. The folding step uses rebinning weights that foldover redundant data at the top and bottom of the fan beam sinogram. The redundant rays are found in the upper left and lower right corners of the sinogram in an intermediate step in rebinning, and each redundant ray corresponds to one ray in the central, non-redundant, part of the sinogram. Weighting is such that the weight of the redundant ray plus the weight of the central ray sum to one, with the sum of the weighted central ray plus the weighted redundant ray replacing the central ray value in the intermediate sinogram. Thus, applicant's fold-over rebinning advantageously uses all of the data from the fan beam X-rays. Applicant's fold-over rebinning technique may be used in single scan CT reconstructions and in multiple scan cone beam correction reconstructions . For cone beam correction reconstructions, the rebinning technique is applied to two scans at once and results in two parallel beam sinograms. Redundant rays from one scan are added to the central rays of the other scan and vice versa using the above rebinning weights. This results in parallel beam sinograms properly prepared for use in applicant's cone beam correction parallel beam reconstruction method. In a second aspect, the present invention provides a fast executing modification of the parallel beam Fourier reconstruction method as described by Tabei. This modification may be used either for reconstruction of single scans or for multiple scan cone beam correction reconstruction. Applicant's reconstruction method first filters the parallel beam data for each view (which has resulted from applicant's modified rebinning algorithm) with a conventional parallel beam kernel, circularly shifts, and then transforms. Next, the transform is replicated and multiplied by an interpolation filter. The thus processed data are then convolved with a gridding function and added into the Fourier image at an angle corresponding to the view angle. After all views have been treated as above, the two- dimensional inverse Fourier transform is taken to yield a preliminary image. Finally, the center of the preliminary image is extracted and multiplied by the inverse of the transform of the gridding function, thus yielding the desired image. The present invention preferably achieves this implementation by using a Kaiser-Bessel gridding function that is precalculated and stored in a table. In a third aspect, the present invention implements cone beam correction reconstruction using the above parallel beam Fourier reconstruction method, whereby cone beam error is substantially corrected. Cone beam error correction requires two or more scans to reconstruct an image. In an n-scan reconstruction, the present invention requires n- scans that are separated along the z-axis by a distance equal to d/(n-l) , where d is the tangent of the cone angle times the reconstruction circle diameter. Data from each scan is weighted during backprojection using a cone beam weight function. By suitably weighting the data, a resultant composite scan that has zero cone beam error is created perpendicular to the z-axis. Preferably, cone beam weighting occurs in the transform domain at the transform backprojection step of the Tabei algorithm. According to the present invention, the cone beam weight functions are approximated by functions having relatively few non-zero points in their Fourier transform. Multiplication by the cone beam weights in the spatial domain is accomplished by convolution by the transform of the weights in the transform domain. This convolution is accomplished by multiplication of the transformed view by each non-zero co-efficient of the transform of the weights, and gridding at a position determined by the co-efficient. Rapid processing is promoted in that the relatively few non¬ zero points require less data processing. The present invention further utilizes a Kaiser-Bessel gridding function, the values for which are pre-stored in a look-up table to expedite processing. The present invention further provides zooming of the reconstructed displayed image, without requiring zooming to be at the image center. Other features and advantages of the invention will appear from the following description in which the preferred embodiments have been set forth in detail in conjunction with the accompanying drawings. BRIEF DESCRIPTION OF THE DRAWINGS FIGURE 1A depicts a fan beam scanning electron beam computed tomography system that includes the present invention; FIGURE IB is a block diagram of reconstruction system hardware, according to the present invention; FIGURE 1C is a more detailed block diagram of hardware implementing a preferred embodiment of the present invention; FIGURE 2A depicts fan beam geometry, and associated measurement coordinates; FIGURE 2B depicts parallel beam geometry, and associated measurement coordinates; FIGURE 3A depicts a modified procedure that provides a foldover step during conversation of fan beam data into parallel beam geometry, according to the present invention; FIGURE 3B depicts in further detail the foldover step using in a fan beam to parallel beam rebinning conversion, according to the present invention; FIGURE 3C depicts the effect of the foldover step depicted in Figure 3B, according to the present invention; FIGURE 3D shows in detail the last rebinning coordinate change, according to the present invention; FIGURE 3E shows a two scan rebinning procedure, including folding over, according to the present invention; FIGURES 4A and 4B depict scan spacing for. a two-scan reconstruction, and associated weighting function, according to the present invention; FIGURES 4C and 4D depict scan spacing for a three-scan reconstruction, and associated weighting function, according to the present invention; FIGURES 4E and 4F depict scan spacing for a four-scan reconstruction, and associated weighting function, according to the present invention; FIGURE 4G depicts an approximation to a four-scan weighting function using seven points in the Fourier domain; FIGURE 5 is a generalized block diagram showing transform backprojection, according to the present invention; FIGURE 6 is a block diagram showing backprojection of transformed views, according to the present invention; FIGURE 7 is a block diagram showing normalization of a reconstructed image, according to the present invention; FIGURES 8A and 8B are fan beam reconstructions showing cone beam artifacts; FIGURES 9A and 9B are fan beam reconstructions with reduction of cone beam artifacts, according to the present invention. DESCRIPTION OF THE PREFERRED EMBODIMENTS Figure 1A depicts a scanning electron beam computed tomography ("CT") system 8 that includes a vacuum housing chamber 10 wherein an electron beam 12 is generated and caused by a beam optics assembly 13 to scan a circular target 14 located within chamber 12's front lower portion 16. Upon being struck by the electron beam, which typically scans 210° or so, the target emits a moving fan-like beam of X-rays 18 that pass through a region of a subject 20 (e.g., a patient or other object) lying within the reconstruction radius R. These rays then register upon a region of a detector array 22 located generally diametrically opposite. The detector array outputs data to a computer processing system 24 that processes and records the data to produce an image of a slice of the subject on a video monitor 26. As indicated in Figure 1A, the computer system 24 may also control the system 8, and includes the present invention 42, MR/TBP, a modified rebinning and transform back projection method whereby cone beam error is substantially eliminated. The system of Figure 1A is a fan-beam system, and provides fan beam data in a fan beam sinogram (or data array) . While fan beam data may be suitably processed using spatial domain algorithms to provide a reconstructed image of an X-ray object, such reconstruction involves many mathematical operations that require custom designed special hardware to implement. Thus, for reasons of processing speed and the ability to use standardized array processing equipment, it is preferred to convert, or rebin, the fan beam data to parallel beam data. Once the data has been suitably rebinned, transform domain backprojection techniques suitable for parallel beam data may be used to reconstruct an image, without requiring specialized processing equipment. Figure IB is a more detailed depiction of hardware implementing the present invention. Data from the CT scanner hardware, e.g., from detectors 22, are received into computer processing system 24 , more specifically into a VME Bus Scan Memory 31. The data are then moved into a VME Bus array processor board 33 that is part of system 24. The array process board preferably uses four to eight standard, commercially available i860 high speed, floating point computational processors that implement the method of the present invention. The i860 array processors are manufactured by Mercury Computer Systems, Inc., located in Lowell, MA. After suitable signal processing according to the present invention, which preferably is stored within computer system 24, a reconstructed image, substantially free of cone beam artifacts, is displayed on monitor 26. Figure 1C is a further detailed depiction of system 8. Figures 2A and 2B depict the relationship between the fan beam sinogram coordinates associated with a system such as that shown in Figure 1A, and parallel beam sinogram coordinates. In the fan beam configuration of Figure 2A, X- rays radiate fan-like from a common source and are detected, after perhaps being attenuated by an object within a reconstruction radius intermediate to the source and detectors. In Figure 2A, the detector(s) lie in a circular arc, similar to what is shown in Figure 1A. In Figure 2A, β is the view angle of the fan center and determines view orientation, while σ is the angle of each ray within each fan beam view, where -A/2≤σ≤+A/2, where A is the fan angle, the maximum angle needed to encompass the entire reconstruction circle of radius R. In the parallel beam configuration of Figure 2B, rays generated by a source are all parallel in one direction and after perhaps being attenuated by an object within a reconstruction radius are detected by detectors lying in a plane parallel to the plane of the sources. In Figure 2B, θ is the angle of the view, and S is the position of the ray within the view, -R≤s≤R, where R is the reconstruction circle radius. Because the present invention is used with a fan beam CT system, it is first necessary to rebin the fan beam data into parallel beam format in order to use a modified parallel beam Fourier technique reconstruction method. Rebinning converts fan beam data having fan beam coordinates (σ,β) into parallel beam geometry that has parallel beam coordinates (s,0) . CT data acquired by a fan beam scanner, such as shown in Figure 1A, is converted by normalization routines into a fan beam sinogram: /(σ,β) ,-^<σ<- ,0<β<π+A. where β is the view angle, σ is the angle within a view, and A is the fan angle. The views cover angles from 0 to τr+A, which is the minimum needed for short scan fan beam reconstruction. It will be appreciated that in a fan beam geometry, each fan ray comes from one parallel view that is parallel to the ray, and vice versa. In essence, rebinning takes such ray and places it into the correct bin in the parallel view. The rebinning algorithm is a two-dimensional interpolation of the input fan beam data that converts the data into parallel beam coordinates: f(s,0) , -R<s<R, 0<0<7τ where θ is the parallel view angle, s is the distance within the view, and R is the reconstruction radius. The relation between the two coordinate systems is given by: θ = β+σ s = Rsinσ. The input fan beam sinogram 50 covers 180° + fan angle, whereas the output parallel beam sinogram 62 covers 180°. The two-dimensional coordinate change is accomplished in two one-dimensional steps. As shown in the sinogram depiction of Figure 3A, the input fan beam sinogram 50 first undergoes a one-dimensional transformation of the columns, step 52, from f { σ , β) to f ( σ , θ ) . The angle between parallel views is chosen to equal the angle between fan beam views. In this case, the transformation on each column is just a shift of the data, which is accomplished by interpolation. This step can be displayed graphically as shown in Figure 3B. In the preferred embodiment, the step size in θ is taken to be equal to the step size in β, whereupon this interpolation amounts to a shift of each column. With reference to the listing of the rebinning algorithm used in the present invention, APPENDIX 1 attached, the input fan beam sinogram 50 has size fansamps • fanviews, where fansamps is the number of equiangular fan beam samples, and fanviews is the number of fan beam views. The rebinning algorithm assumes that the fan views cover 180 degrees plus the fan angle A. APPENDIX 1 is believed to be sufficiently annotated as to be readily understood by one skilled in the relevant art. To the extent any of the nomenclature in APPENDIX 1 may differ from what is set forth in the Specification text, such differences will be readily apparent to those skilled in the relevant art . After the rebinning column transformation step 52, the resulting intermediate £ ( σ , β ) sinogram contains more data than is strictly necessary for a parallel beam reconstruction. More specifically, the central rectangular portion 54 holds all the data necessary for a parallel beam reconstruction. The data in the triangular portions 54A, 54B are redundant. By this it is meant that the spatial position of a ray in 54A determined by the angles ( σ , θ ) is the same as the position of the ray determined by the angles ( - σ , θ+ττ) . That ray will fall inside the central rectangle 54. Similarly a ray in the triangle 54B at (σ 1 ,θ 1 ) has the same position as { - σ χ , θ 1 -ιt) , which is in the central rectangle 54. Thus the data in the corner triangular regions 54A and 54B may be discarded or, more preferably, folded into the central rectangle. At step 56, foldover occurs, whereby the redundant data in the corner triangles 54A, 54B are folded into the main sinogram 54, resulting in the sinogram shown in Figure 3C. In one aspect of the present invention, applicant has discovered that it is possible to create foldover weights, for use at step 56, using formulae known in the art for use with short scan fan beam reconstruction. Applicant's rebinning weights are calculated in the same manner that weights were determined for a short scan fan beam algorithm (wherein no rebinning occurs) as described in the Dennis Parker reference, cited earlier herein. The use of such weights for rebinning as disclosed herein is believed new. The rebinning used with the present invention is especially advantageous in providing a convenient processing step whereat to insert a folding step 56. Further, a multiple scan data foldover step disclosed herein is required to both correct cone beam error and permit reconstruction using parallel beam techniques. As will be described, foldover 56 is required for subsequent cone beam error correction. Folding over makes full use of all data obtained from a radiated object, and improves the signal-to-noise ratio in the reconstructed image, as viewed on display 26. Further, when acquired from a fan beam system, not all of the redundant data in sinogram 54 are collected in the same plane, due to the Δz error noted earlier, which error gives rise to cone beam artifacts when reconstructing the image. To do cone beam reconstruction according to the present invention, applicant's modified cone beam algorithm makes use of two or more fan beam scans to create one image, thus making it necessary to rebin on two or more scans. Rebinning on a single scan would not yield the desired reconstruction, although a foldover step using data from a single scan would still help reduce cone beam artifacts for that one scan. For a cone beam reconstruction that requires n scans the rebinning algorithm of the present invention proceeds on pairs of scans as follows. The first scan is paired with scan n, the second with the scan n-1, and so on. If n is odd the middle scan will not have a pair. This scan is then rebinned by itself and the folding is done into itself. In the present invention, the corner areas of one scan require folding into the central area of the other scan, in which case the rebinning algorithm performs rebinning on both scans at once. At the folding step, e.g., step 56 in Figure 3A, the rebinning algorithm folds the corner areas of the first scan into the main portion of the second scan and vice versa. Figure 3E depicts two scan cone beam rebinning, wherein input data from two fan beam sinograms acquired a small distance Δz apart are rebinned simultaneously, with the rebinning output being two parallel beam sinograms. In Figure 3E, step 52-A denotes column interpolation for the data of the first scan, whereas step 52-B denotes column interpolation for the data of the second scan. Returning to Figure 3A, in step 56, in general folding is accomplished by weighting each central point and corresponding corner point or regions 54A, 54B, using weights derived from those used in short scan fan beam reconstruction. The weight used as a co-efficient for the sinogram corner of one scan, and the weight used as the coefficient for the sinogram center of the other scan always add to one. Thus weighted, the sinogram corner of one scan is added to the sinogram center of the other scan. According to the present invention, by doing the foldover step 56 as shown in Figure 3E, after the first one- dimensional interpolation, a further interpolation is avoided. A sinogram does not consist of an infinite number of points, but rather a finite number of points at discrete positions. The positions are so chosen that if the coordinates (σ,0) fall exactly at a data point present in the sinogram then the coordinates ( - σ , θ+ιτ) or (-σ,0-τr) will also fall exactly on a point present in the sinogram. Thus interpolation between two points is not necessary in the folding step. This is not the case if the folding step were done on the sinogram at stage 50 or 62 in Figure 3A. For an actual fan beam CT scanner as shown in Figure 1A, for example the C-150 model manufactured by Imatron, Inc., of So. San Francisco, California, data in corners 54A, 54B are not truly redundant. Due to the cone beam geometry of this scanner, the corner rays have a slightly different orientation than the corresponding central rays. After foldover step 56, the resultant sinogram 58 undergoes a final rebinning step 60 that results in a row transformation from f(σ,0) to f(s,0), resulting in the parallel beam sinogram 62. In step 60, each row is interpolated from (σ,0) coordinates into parallel beam geometry having parallel beam coordinates (s,0) . With further reference to Figure 3A, this second coordinate change 60, from σ to s is done on each row of the f(σ,0) sinogram 58 using the equation s = Dsinσ, where D is the distance from the X-ray source to the detector. This second coordinate change is accomplished by a straight forward interpolation of each row, and is depicted in Figure 3D. The vertical lines in Figure 3D indicate that lines equally spaced in s do not fall an equal distance apart in the sinogram 58, but are converted by step 60 to sinogram 62 in which they are an equal distance apart . According to the present invention, interpolations are used repeatedly in the rebinning process. The general interpolation algorithm may be described as follows: Let there be a function f(i) defined on integer points, where it is desired to find the interpolated value of f at a point x where 0<x<l. This value of the function f (i) is calculated from the formula: m<ni f (x) = Σ f (m)I(x-m) m=-ni where I (x) is the interpolation kernel, and ni is the order of the interpolation. An interpolation of order ni will use 2ni points of the original function for each output point. In the present invention, the interpolation kernel used in the rebinning interpolations is a sine function, (sin TΓX) /πx, tapered by a Gaussian, where the kernel size may be any length n: I (x) = sine (x) -exp- (x 2 /ni) In practice, this function is slightly modified in that the values of I (x) are scaled so that for all x, O≤x≤l: m<ni Σ I(x-m) = 1 m=-ni At this juncture, the original fan beam data have been transformed into a parallel beam sinogram of size nsamps x nviews, where the number of samples per view is nsamps, the number of views is nviews, and where the set of views covers 180°. View v will represent a parallel projection at angle vangle = v-180/nviews. It will be assumed that nr is the least power of two greater or equal to nsamps. The following describes the preparation of each view prior to backprojection using applicant's parallel beam backprojection modified Fourier technique, which is a modification of prior art gridding type techniques. By suitably modifying and combining features from these various techniques, the present invention is able to correct cone beam error in a fan beam CT system, using Fourier methods. According to the present invention, applicant's modified algorithm, a Tabei type transform backprojection algorithm, has the following process steps, as shown in Figures 5-7. Figure 5 gives an overview of the process . Figure 6 gives details of Figure 5 step 80. Figure 7 gives details of Figure 5 step 100. The input to the process is a set of n parallel beam sinograms, each sinogram consisting of a set of views. For each of the n sinograms there is a different cone beam weight function. In the case when n is one then no cone beam correction is done. (1) for each view, the parallel beam data (which has resulted from applicant's modified rebinning algorithm, is convolved with a conventional parallel beam kernel (Figure 6, step 120) , e.g., see APPENDIX 1, p. 17, executed by subroutine kerconv) ; (2) the result of step (1) is then circularly shifted by an amount equal to half the view width and transformed (Figure 6, step 122, e.g., see APPENDIX 1, p. 18, executed by subroutine cshift) ; (3) the result of step (2) is then replicated by complex conjugate folding and multiplied by an interpolation filter (Figure 6, step 124, see APPENDIX 1, p. 18, subroutines rfft, foldview and vmul) ; (4) in the case of an offset reconstruction the result of step (3) is multiplied by shift coefficients (Figure 6, step 126) ; (5) for each non-zero coefficient in the transform of the cone beam weight function associated with the sinogram multiply the result of step (4) by the coefficient and sum the result for all input sinograms (Figure 6, step 128) ; (6) convolve the result of step (5) with the gridding function and add into the Fourier image at an offset determined by the weight coefficient number and along an angle corresponding to the view angle (Figure 6, steps 130 and 132) ; (7) after steps (5) and (6) are repeated for each non-zero weight coefficient and steps (1) through (6) are repeated for all views, take the two dimensional inverse Fourier transform to get a preliminary image (Figure 5, step 90) ; (8) Finally, for such preliminary image extract the central region and multiply by the transform of the gridding function, then scale and fix to integers to get the desired reconstructed image (Figure 5, step 100 and Figure 7, steps 150, 152, 154, e.g., see APPENDIX 1, subroutine fbackpdb used for normal cone beam case) . Briefly, the cone beam correction method of the present invention is analogous to a weighting scheme for each backprojected view, wherein a two-dimensional weighting function is calculated for each view that gives the contribution (weighted 0 to 1) of that view to each pixel in the image. Preferably the two-dimensional weighting function is approximated by a function whose two-dimensional Fourier transform consists of a small number of non-zero terms, to promote speed of execution. Multiplication of the back-projected view by the two- dimensional weighting function may then be done in the transform domain as a convolution step. The reconstructed image is built-up by summing for each view the backprojection of the view times that view's weighting function. According to the present invention, the weighting function is simplified by requiring that the scans be interpolated into scans that are perpendicular to the z axis (ignoring the cone angle) . Such scans will be denoted z-perp scans. A z-perp scan would result, for example, if the system of Figure 1A were used to make a scan while the patient was stationary, and then the patient were moved along the z-axis relative to the scanner, at which point another scan were made. For such a method of scan acquisition, the two-dimensional cone beam weighting functions approximate a one dimensional function parallel to the view angle. In an alternate method of scan acquisition, called spiral scanning, the patient is continuously moved while the scanning takes place. The scans thus acquired are not perpendicular to the z-axis and are interpolated to z-perp scans before reconstruction with the present invention. A transformed backprojection fan beam image is reconstructed from n z-perp scans, where number n and spacing of the z- perp scans is governed by the slice width, cone angle, desired reconstruction circle radius R, and position of the desired images. Interpolation from spiral scan to z-perp scan is straightforward, and each point in the z-perp fan beam sinogram is interpolated linearly from the corresponding points in the nearest spiral scans. If desired, a higher order interpolation may be used. Figures 4A and 4B depict z-perp scan spacing and associated weighting functions for a two scan cone beam reconstruction (e.g., two fan beam scans used to reconstruct a single image) , while Figures 4C, 4D and 4E, 4F are similar depictions for three-scan and four-scan reconstructions, respectively. In Figures 4A, 4C, 4E, there is shown in a vertical phantom line the central rays for one view in each of the two, three and 4 z-perp scans used to create the image whose position is indicated by the dotted line. The inclination of each ray represents the undesired offset in planes defined by the source of the X-ray radiation and by the detectors. By definition, the phantom vertical line has zero offset, and if such a ray actually existed, would represent the desired zero cone beam error condition. In essence, the phantom vertical lines represent a backprojected ray formed as the weighted sum of rays from each scan, which ray does lie in a co-incident plane. The distance, z d , between z-perp scans is given by z d =d/(n-l) where d is the cone beam distance defined by d=tan(cone angle) •2R where n is the number of z-perp scans in the image, and R is the reconstruction radius. In the case of a 2 scan cone beam correction (Figures 4A and 4B) , the algorithm will linearly weight each backprojected view in the projection direction with weighting varying from 0 to 1 for the first scan and from 1 to 0 for the second scan. This is done during transform backprojection in the frequency domain by convolving the transformed view with the transform of the weighting function. In this case, a very simple weighting function may be chosen: a sinewave having but two terms in it's Fourier transform. By zooming in on a small portion of the sinewave near the zero crossing, applicant can synthesize a weighting function that is very nearly linear. The determination of n, the number of scans input to the cone beam correction, depends on the slice width of each scan, the desired slice width for the image, and the distance d. As a minimum, n should be chosen sufficiently large so 2d is smaller than the scan slice width. Larger n will create an image with a more constant slice width, which will approach the scan slice width as n is increased. The weighting functions, shown in Figures 4B, 4D, 4E for the two, three and four-scan images, are one-dimensional functions that describe the two-dimensional weights applied to the backprojected parallel beam view. The same weight function is applied to all views in a z-perp scan. The weight is applied to the backprojected pixels as a function of distance from the reconstruction circle perimeter measured along the view angle. Consider, for example, the weighting functions of Figure 4B. At sweep 1, ray position Al (Figure 4A) , the data will be perfect because the ray is precisely upon the vertical phantom line position. Therefore the weighting co-efficient is 1 at that position (Figure 4B, position Al) . However for that same ray in sweep 1, as position A2 is reached, the ray goes farther from the ideal vertical position, and accordingly it is given less weight, until at position A2 is given zero weight (see Figure 4B) . Consider the ray for the second sweep. At position Bl the ray is far from the ideal location, and Figure 4B indicates that its weight co-efficient is accordingly zero. However at position B2, the ray is precisely on the vertical phantom position, and its co-efficient is 1 (Figure 4B) . By so weighting the rays from sweep 1 and sweep 2, a pseudo-ray having a zero cone beam error position corresponding to the dotted phantom line may be deemed to have been created. In similar fashion, appropriate weights are depicted in Figures 4D and 4F for three and four scan reconstructions, although more than four scans may be used. These functions used to weight the backprojected views are preferably implemented as a convolution in the transform domain. Since the speed of backprojection varies directly with the number of points in the transform, it is advantageous to approximate the weighting functions with functions requiring fewer transform points. Figure 4G, for example, is a plot of an approximation to a four scan reconstruction weighting function using only seven points. Figure 5 is a generalized block diagram of the present invention, wherein rebinning including steps 52, 56 and 60, as above described, occur first. At process step 80, backprojection of the thus transformed views occurs, and at process step 90, the two-dimension inverse fast Fourier transform of the image is taken, the image being normalized at step 100. Turning now to Figure 6, backprojection of transformed views according to the present invention is depicted. Each view in a parallel beam sinogram is processed as shown in Figure 6, and then added into a two-dimensional Fourier transform. Figure 7 provides further detail as to the image normalizing process step 100, shown in Figure 5. The method steps shown in Figure 6 will now be described in further detail . The steps depicted in Figure 6 are applied to each view in the parallel beam sinogram. In the case of a cone beam scan, there will be two or more parallel beam sinograms that are processed together. Each view will consist of rebinned projection data of length nsamps, with a parallel view angle of vangle, the angle corresponding to angle 0 in Figure 2B. As noted, the view must be filtered by a parallel beam kernel (Figure 6, step 120) . Preferably this is done by forward transformation, multiplication in the Fourier domain by the transform of the kernel, then inverse transformation. The size of the Fourier transform is 2«nr real points, and the view is padded with zeros to this size. Next, the convolved view is circularly shifted by nsamps/2 and padded to length nr, see Figure 6, step 122. A real Fourier transform is then performed to get an nr/2 + 1 length complex vector representing the positive part of the Fourier transform of the convolved view. The thus transformed view is replicated by folding with conjugation about the nr/2 term producing a nr + 1 point complex vector, f(nr/2+i) = f(nr/2-i)*, i = 1, ..., nr/2, Figure 6, step 124. In practice, the high frequency i = nr term may be discarded, and term 0 is divided by 2. The replicated view is multiplied by an interpolation filter that may be used to tailor the interpolation frequency response (Figure 6, step 124) . For example, for linear interpolation the filter is sine (r-τr/nr) 2 , r = 0, ..., nr-1. For a response closer to cubic interpolation, the filter is [8 + 9 -cos (τr-r/nr) - cos (3 •π-r/nr) ] /16 The view at this stage will be called the transformed view, rather than the convolved, shifted, transformed, replicated, filtered view. The present invention advantageously permits an off-center image reconstruction by using the Fourier shift theorem to perform a shift in the transform domain (Figure 5, step 100, Figure 6, step 126, Figure 6. The basis of this algorithm is that the parallel beam sinogram, when transformed, becomes a polar coordinate version of the two-dimension fast Fourier transform of the image. Thus, to shift the image, the Fourier shift theorem can be applied to the transformed view. Assume that shifts of coordinates sx, sy are desired, where the units are such that there are nr units in the reconstruction radius R. The nr complex points in the view are at positions [x(r),y(r)] = [r• -cos (vangle) , r-sin(vangle) ] , r = 0, ..., nr-1. These points are complex multiplied by - (2-τr-i- (sx'x(r) + syy(r) ) /nr] Next, the backprojection of the view is done in the transform domain. The transformed view is convolved with the gridding function and added into the transform of the image. The image is an nf-nf real image, with transform represented as nf/2-nf complex terms. Backprojection according to the present invention entails providing coordinates for each point in the transformed view, using a gridding function that preferably is a Kaiser-Bessel function whose values are pre-stored in a look-up table, convolution with the gridding function, then addition of the gridded view into the Fourier domain image at positions determined by the coordinates. In the case of a cone beam correction the backprojected view is multiplied by a weighting function. This is accomplished by convolution of the transformed view with the transform of the weight function. This convolution is accomplished by multiplying the transformed view by each non-zero coefficient of the transform of the weight function, and then gridding at coordinates offset from the view coordinates. More specifically, with respect to the view coordinates, each complex point in the transformed view is given the coordinates : (u(r) ,v(r)) = (-r-reconr-2 -cos (vangle) , sin(vangle) ) where r = 0, ...,nr-l. Reconr is the fraction of the reconstruction radius R to be covered by the scan. Reconr = 1.0 results in a image covering the whole reconstruction circle, whereas reconr = 0.5 results in an image covering half of the reconstruction circle, i.e. a zoom of 2. The point is to be multiplied by the gridding function and added into the image at points centered at the image coordinate. The choice of angle [cos (vangle) , -sin(vangle) ] in the Fourier image produces a backprojection angle of [-sin (vangle) , -cos (vangle) ] in the spatial image, where the y direction is positive measured downward. Since the coordinate calculation depends on cos (vangle) and sin(vangle) , symmetries of these trigonometric functions can be used to reduce calculations. The coordinates are calculated for four views at once: the views at vangle, 7r-vangle, vangle+7r/2, and 7r/2-vangle. Relations between the sines and cosines of these angles allow a reduction in calculation by a factor of two. The gridding function is preferably a small, separable two- dimensional real function whose width is given by the variable nt . Preferably the gridding function is a Kaiser-Bessel function with shape governed by a parameter β: cf(x) = besseliO (βV(1.0 - w(x) ) /besseliO (β) w(x) = (2-x/nt) 2 -nt/2 < x < nt/2, cf (x) = 0 elsewhere. As shown in Figure 7, step 150, next each point of the transformed view, fv(r) is multiplied by the gridding function and added into the Fourier image, fim(iu,iv) using the formula: fim(iu,iv) = fim(iu,iv) + cf (iu-u (r) ) •cf (iv-v(r) ) •fv(r) The gridding function is zero except for an nt x nt square around the position (u(r) ,v(r)) . Thus, this method step consists of determining the nt-nt values of the gridding function for the position (u(r) ,v(r)) , multiplying the values by fv(r) , and then adding them into the image. The gridding function is separable so only 2nt values must be determined. These values depend on the fractional errors ceil(u(r)) - u(r) , and ceil(v(r)) - v(r) . Rather than calculate the gridding function each time, the present invention pre-calculate a table of values indexed by quantized fractional errors . With respect to Figure 1A, the look-up table storing these values preferably is associated with computer system 24. A table size nq = 1024 appears sufficient, in which case the table will contain nt entries for each q, q = 0, ..., nq-1: table [q,j] = cf (q/nq + j - nt/2) , j = 0, ..., nt-1. The variable's governing a two scan cone beam backprojection will now be described, with reference to the attached APPENDIX 1, which lists the relevant code. val, va2 are the first and second weighting angles, val = vangle + TΓ if vangle < ττ/2, and val = vangle if vangle ≥ 7r/2 va2 = vangle if vangle <τr/2, and va2 = vangle + τ if vangle > ττ/2. cbscale is the slope of the weighting = reconr/coner. A slope of one means that the weighting goes from 0 at +reconr to 1 at -reconr. cbdistO is the default value for cbdist, the parameter that determines the amount of zooming in on the sinewave. cbdist is the distance in Fourier image coordinates between 0 and the positive term of the sinewave expansion. cbdist = cbdistO •cbscale. cbmult is a needed scale factor: cbmult = .5/sin(cbdistO •7τ/2) . tsh is an angular shift, different for each scan, that specifies the desired part of the sinewave. tshl = cbdistO -7τ/2 • [1.0 + cbscale• (sin(val) -x0 + cos (val) -y0) ] tsh2 = cbdistO • τr/2 • [1.0 + cbscale• (sin(va2) -xO + cos (va2) -y0) ] cbcoeff is the complex coefficient of the Fourier representation of the sinewave. cbcoeffl = (cbmult -sin (tshl) , -cbmult •cos (tshl) ) cbcoeff2 = (cbmult -sin(tsb.2) , ÷cbmult•cos (tsh2) ) Consider now the cone beam backprojection, where viewl is the transformed view of the first scan, and view2 is the transformed view of the second scan. First, viewl is multiplied by cbcoeffl, and view2 is multiplied by cbcoeff2. Next the results are added and then backprojected at the points (sin(val) -cbdist + u(r) , cos (val) •cbdist + v(r)) , r = 0, ... , nr-1. C o o r d i n a t e s ( u ( r ) , v ( r ) ) r-reconr ■ 2 • [cos (vangle) , -sin(vangle) ] , where r = 0, ..., nr-1, and where reconr is the fraction of the reconstruction radius R to be covered by the scan Next cbcoeffl and cbcoeff2 are conjugated, the two views multiplied and added as above, and then backprojected at the points (-sin(val) -cbdist + u(r) , -cos (val) •cbdist + v(r)) , r = 0, ... , nr-1. Although a preferred implementation reconstructs cone beam data using two scans, more than two scans may instead be used, in which case more sophisticated weighting functions must be synthesized. In Figure 4B, for example, the weighting functions for a two scan correction are a negatively sloping ramp going from 1 to 0, and a positively sloping ramp going from 0 to 1. It follows, then, that the weighting functions needed for a four scan cone beam correction will have the downward slope of scan 1 in Figure 4D, the triangular slope of scan 2 in Figure 4F, the once-delayed increasing slope of scan 3 in Figure 4D, and the twice-delayed slope of scan 4 in Figure 4F. Such shapes can be approximately synthesized by using several terms in the Fourier transform of the weighting function. Next, the gridded view is added into the Fourier image. The Fourier image, fim(iu,iv) is defined for iu = 0, ..., nf/2, iv = 0, ..., nf-1. In the fim(iu,iv) gridding formula noted above, iu and iv may range over all integers but are then mapped into the Fourier image modulo nf, i.e. iu = iu % nf, iv = iv % nf. If iu > nf/2, then iv is replaced by nf-iv, iu is replaced by nf-iu, and the value of the term is conjugated. Inverse transformation and normalization of the image next occurs, Figure 5, steps 90 and 100. After backprojection of all views, the Fourier image is formatted to conform to the packing convention of the fast Fourier transform software used with the present invention, and is inverse transformed. The resulting image is then divided by the transform of the convolving function. This transform is calculated as follows. First, a complex function is created using the formula: c(i) = (cf(i) , 0) i = 0, ..., nf/2-1.. This function is inverse transformed to get a real function w(i) , i = 0, nf-1. Then n(i) = V (scale) /vr (x) is formed. Finally, the image point im(i,j) is multiplied by n(i) -n(j) . Only the center nf/2-nf/2 portion of the resulting image is used (Figure 7, step 152) , and preferably is fixed to 16 bit integers (Figure 7, step 154) . Having described the preferred embodiments, Figures 8B and 9B depict the improvement resulting from use of the present invention, when compared to respective Figures 8A and 9A. The images of Figures 8A, 8B, 9A and 8B were taken from an Imatron model C-150 fan beam scanner, having 6 mm slice thickness, and show a 13 cm reconstruction radius. Figures 8A and 9A are two uncorrected images of a rib phantom, wherein image reconstruction was made using a prior art fan beam algorithm. Note the cone beam error in Figures 8A and 9A, manifested by shadowing behind the rib, which appears in white. By contrast, Figures 8B and 9B show an image from the same scanner, after processing by the present invention. Two z- perp scans were used to create the images of Figures 8B and 9B, with 3 mm separation between scans. Note the reduction in cone bean error in these figures when compared respectively to Figures 8A and 9A. The rib, in white, has substantially no cone beam shadow artifact. For fan beam data acquired from an Imatron model C-150 scanner, execution time for the present invention running on a single 860 processor is presently approximated by: T = 7.5-Nscans + 9.8Npoints + 1.5 where Nscans is the number of z-perp scans used in the reconstruction, N points is the number of complex points used in the Fourier transform of the weighting function. For example, for a two scan cone beam scan, and a two point weighting function, T <= 36.1 seconds. Of course, this run time may be cut by a factor of four by executing on a quad 860 processor board. Modifications and variations may be made to the disclosed embodiments without departing from the subject and spirit of the invention as defined by the following claims. /* * File Name: trecMain.c * * Author : Jon Harman * Brief Description: Imatron TBP reconstruction main program. * Copyright 1993 Imatron, Inc. * * Command Line Synopsis: * Long Description: * Deficiencies / bugs: * Return (status) codes, error messages: * * Abbreviations used: * * Revision History (latest updates first!): 3/12/93(jonh) New. */ /* 1.) "Imported" data types and defines: */ /* l.a.) Standard C include files */ ♦include <stdio.h> ♦include <math.h> ♦include <string.h> ♦ifndef CSPI ♦include <sys/types.h> fendif /* l.b.) Imatron ../include files */ ♦include " ../include/imatron.h" /* first Imatron include */ ♦include "../include/scanner_config.h" /* scanner config */ /* I.e.) Project include files */ ♦include "trec.h" /* 1-d.) Other include files */ /* 2.) Externals defined in this file (declarations only): */ FORWARD VOID main() ; /* 3.) "Imported" externals: */ /* 3.a.) Imported from standard C Library */ IMPORT CHAR *malloc() ; IMPORT REAL atof() ; ♦ifdef MC860 FORWARD FILE *pu_fopen() ; ♦else IMPORT FILE *pu_fopen() ; ♦endif /* 3.b.) Imported from ../xxxxx */ /* 3.c.) Imported from other files in this dtrectory */ /* 3.d.) Imported from elsewhere */ /* 4.) "Private" data types, defines, data and code */ EXPORT INT debug = 0, test = 0; /* Help Message for this Program */ PRIVATE STRING HelpLines[] = { "Usage: tree [Options | Parameter values]", ■ Options: ", -h for this message", -clOO 100ms reconstruction (default)", -c50 50ms reconstruction", -test test recon 1", -d for debug mode", -q for quiet mode", -u for non-interactive mode", -cb for two scan cone beam recon", -nfd for no folding of sinogram", -ncf for no corner filling of sinogram", -si (smooth interp if fr < 1)", -zo to zero out areas outside of recon circle", 'Input Options: ", -ps use parallel normalized sinogram for input", "Output Options:", -ss output filled in fan beam sinogram", -sp output rebinned (parallel) sinogram", -sc output convolved projections", -st output transformed views", -sf output Fourier image", -εm output M format Fourier image", -sr output real image", -sn output center of normed real image", "Parameter Values: (note space before value)", -f input (name of input fan beam sinogram) ", -f2 input2 (name of second input fan beam sinogram) ", -o output (name of output file)", -ker kernel (kernel number)", -r fractional recon radius (0 to 1)", -cr fractional cone beam radius (0 to D", -re dia of recon circle (cm)", -s scale (scale factor for image)", -i interpolation type (0=linear, 2=cubic)", -rot rot (image rotation)", -nv nviews (fan beam views over 360)", -ns nsamps (number of samples per view) ", -fa fan angle (deg)", -rw rwidth (parallel width after rebinning) ", -iw output image width", -nt convolution width", -nq kb table size", -b beta for gridding fen", -xO x center of output image (-1 to 1)", -yO y center of output image (-1 to 1)", -ac constant added to image", -el clip2d (parameter for 2D clipping)", -fr radius of radial frequencies(0 to 1)", -gr transition from first to second gridding fen", -gw half width of transition", -nl set rebinning nl", -nk set rebinning nk", -sk skip fanbeam views", -fl 1/0 flip image", -npv number of phantom views", -cfb cfblim", -cfs cfslim", (STRING) NIL /* NIL terminator! */ 3; /* Function to Print Out Help Message */ PRIVATE VOID PrintHelp{) { STRING *LineP; /* Print Lines up to NIL terminator */ for (LineP = HelpLines; *LineP; LineP++) (VOID) printf("%s\n", *LineP) ; } /* 5.) Exported Functions and Data: */ /* MAIN PROGRAM */ /* ARGSUSED *//* < ARGSUSED is for "lint" */ EXPORT VOID mai (argc, arg ) /* entry point of program. */ INT argc; /* Number of arg strings, 1 or more */ STRING argv[] ; /* Address of array of ptrs to arg. strings INT i, j, k, err = 0, orig, half, recontype = MS100, dorebin = 1; INT viewsread, minviews, nl, nsamps, minviewsl; INT v, vO, vl, skip = 0, noni = 0, doagain = 0; INT savef = 0, savep = 0, savet = 0, savec = 0, saver = 0, saveflg = 0; INT quiet = 0, saven = 0, saves = 0, εavem = 0; CHAR str[100) , outfile[80], infile[80], fname[80], infile2[80] ; REAL reconc = -1.0, fr = -1.0, btemp; REAL32 tottim = 0.0, stim, timl, tim2, tim3, tim4, tim5; FILE *fp; TREC_PARAMS trecParams; TREC_TABLES trecTables; TREC_MEMORY trecMemory; ♦ifdef CSPI rtc_start_ () ; ♦endif /* do initializations and set up defaults */ outfile[0] = 0; infile[0] = 0; /* initialize trecParams for 100ms recon */ recontype = MS100; /* parse the command line */ for (i = 0; i < argc; i++) { if (!strcmp(argv[i] , "-h")) { -h should always give help message.. PrintHel () ; exit(0) ; } if (!strcmp(argv[i] , "-d") debug = 1; if (!strcmp(argv[i] , "-da")) doagain = 1; if (!strcmp(argv[i] , *-q")i quiet = 1; if ( !strcmp(argv[i] , "-ps" dorebin = 0; if { !strcro (argv[i] , "-sp" savep = 1; if ( !strcmp(argv[i] , "-sc" savec = 1; if ( !strcmp(argv[i] , "-st" εavet = 1; if ( !strcmp(argv[i] , "-sf" εavef = 1; if ( !strcmp(argv[i] , "-sm" savem = 1; if (!strcmp(argv[i] , "-ss" saves = 1; if ( !εtrcmp(argv[i] , "-sr" εaver = 1; if (!strcmp(argv[i] , "-sn" saven = 1; if ( !strcmp(argv[i] , "-t") test = 1; if ( !strcro (arg [i] , "-cl00")) recontype = MS100; if (!strcmp(argv[i] , "-c50")) recontype = MS50; if ( !strcmp(argv[i] , "-test")) recontype = TESTR1; /* * initialize trecParams for recon before reading the command line * changes */ ini tparams (recontype , fctrecParams ) ,- for (i = 0; i < argc; i++) { if ( ! strcπrp (argv[i) , "-nfd" ) ) trecParams.dofold = 0; if (!strcmp(argv[i] , "-ncf")) trecParams.docf = 0; if ( !strcmp(argv[i] , "-zo")) trecParams.zout = 1; if (!strcmp(argv[i] , "-cb")) { trecParams.cb = 1; trecParams.nq = 2048; ) if ( !strcmp(argv[i] , "-si")) trecParams.si = 1; } for (i = 0; i < argc - 1; i++) { if ( !strcmp(arg [i] , "-re")) reconc = atof(argv[i + 1]); if (!strcmp(argv[i] , "-r")) trecParams.reconr = atof(argv[i + 1] ) ; if (!strcmp(argv[i] , "-cr")) trecParams.coner = atof(argv[i + 1] ) ; if (!strcmp(argv[i] , "-c")) trecParams.cutoff = atof(argv[i + 1] ) ; if (!strcmp(argv[i] , "-b")) trecParams.beta = atof(argv[i + 1]); if (!strcmp(argv[i] , "-eck")) trecParams.eck = atof(argv[i + 1] ) ; if (!strcmp(argv[i] , "-eel")) trecParams.eel - atof(argv[i + 1]); if (!strcmp(argv[i] , "-rk")) trecParams.rk = atof(argv[i + 1]) if ( !strcm (argv[i] , "-rl")) trecParams.rl = atof(argv[i + 1]) if (!strcmp(argv[i] , "-x0")) trecParams.xO = atof(argv[i + 1]) if (!strcmp(argv[i] , "-y0")) trecParams.yO = atof(argv[i + 1]) if (!strcmp(argv[i] , "-xo")) trecParams.xO = atof(argv[i + 1]) if (!strcmp(argv[i] , "-yo")) trecParams.yO = atof(argv[i + 1]) if (!strcmp(argv[i] , "-fa")) trecParams.fanang = atof(argv[i + 1]) * PI / 180.0; if (!strcmp(argv[i] , "-iw")) trecParams.iwidth = atoi(argv[i + 1] ) ; if (!strcmp(argv[i] , "-i")) trecParams.itype - atoi(argv[i + 1] ) ; if (!strcmp(argv[i] , "-ac")) trecParams.ctconst = atof(argv[i + 1]); if (!strcmp(arg [i] , "-s")) trecParams.scale = atof(argv[i + 1] ) ,- if (!strcmp(argv[i] , "-rw")) trecParams.rwidth = atoi(argv[i + 1] ) ,- if {!strcmp(argv[i] , "-nt")) trecParams.nt = atoi(argv[i + 1] ) ; if (!strcmp(argv[i] , "-nq")) trecParams.nq = atoi(argv[i + 1] ) ,- trecParams.nq = 2048; } if (!strcmp(argv[i] , "-ker")) trecParams.ktype = atoi(argv[i + 1] ) if ( !strcm (argv[i] , "-nk")) trecParams. k = atoi(argv[i + 1]); if (!strcmp(argv[i] , "-nl")) trecParams.nl = atoi(argv[i + 1] ) ; if (!strcmp(arg [i] , "-sk")) skip = atoi(argv[i + 1]); } /* now that we have our options do some calculations based on them */ /* 47.5 is assumed to be max recon diam in cm. */ if(reconc > 0.0) trecParams.reconr = reconc / 47.5; trecParams.iwidth = (trecParams.iwidth / 2) * 2; /* make even */ /* usually iwidth equals fwidth/2. If not reconr needs to be adjusted so that iwidth represents a recon radius of 1 */ if(trecParams.iwidth != trecParams.f idth / 2) trecParams.reconr *= .5 * (REAL) trecParams.fwidth / (REAL) trecParams.iwidth,- /* fr is the radius in Fourier space that we bac project over. It should equal cwidth/2 for full bandwidth. If it is set lower some smoothing may be noticible if εi = 1, ringing if si = 0. However if the original data does not have high frequencies fr can be set lower with si = 0 and little ringing will occur. Setting si = 0 and fr = .5 seems to work well for cl50 data. This seems to avoid "fingerprint" artifacts associated with keeping the high frequencies. So far no ringing has been noticed. /* if fr > 0 user wants to set it */ if(fr > 0.0) trecParams.fr = trecParams.cwidth * fr * .5; else /* when iwidth < fwidth/2 some smoothing is helpful */ if(trecParams.reconr > 1.0) trecParams.fr /= trecParams.reconr; if( (trecParams.gridr > 0) && (trecParams.fr < trecParams.gridr + trecParams.gridw) ) trecParams.fr = trecParams.gridr + trecParams.gridw; if(trecParams.fr > trecParams.cwidth / 2) trecParams.fr = trecParams.cwidth / 2; trecParams.fr = (trecParams.fr / 2) * 2; /* make even, needed by spreads */ trecParams.gridr = (trecParams.gridr / 2) * 2; /* make even */ trecParams.gridw = (trecParams.gridw / 2) * 2; /* make even */ if(trecParams.fr < 2) trecParams.fr = 2; if(savec) saveflg += SAVEC;/* tell tbp to save convolved εino */ if(savet) εaveflg += SAVET;/* tell tbp to save transformed sino */ if(!trecParams.docf) { trecParams.npviews = 0; trecParams.cfblim = 0; trecParams.cfslim = 0; } /* * Do the setup's needed. */ trecTables.memtot = 0; trecMemory.memtot = 0; tmr_εtart_timesec() ; if(dorebin) { /* create the tables and constants needed for rebinning */ err = trecRBTable(&trecParams, ttrecTables) ; if (err) { printf("tree: Error:%d when setting up RB tables.\n", err); exit(l) ; } ) /* create the tables and constants needed for convolution and backprojection */ err = trecTBPTablef-itrecParams, fctrecTables) ; if (err) { printf("tree: Error:%d when setting up TBP tables.\n", err); exit(l); ) /* allocate the memory needed */ err = allocmemt&trecParams, fctrecMemory, dorebin); if (err) { printf("tree: Error:%d when allocating memory.\n", err) ,- exit(l); ) if(test) { if(trecParams. t == 5) { printf( • *** Special test mode nt 5 -> 3. norm with 5\n"); btemp = trecParams.beta; trecParams.beta = 10.3; APP make_imgwint&trecParams, trecTables.imgwin) ; trecParams.beta = btemp; for(i=0;i<trecParams.nq;i++) { trecTables.grtable[i * 5) = 0.0; trecTables.grtable[i * 5 + 4] = 0.0; } } if(trecParams.nt -- 3) { printf("*** Special test mode nt 3 norm with 5.\n"); trecParams.nt = 5; btemp = trecParams.beta; trecParams.beta = 10.3; make_imgwin(fctrecParams, trecTables.imgwin) ; trecParams.nt = 3; trecParams.beta = btemp; } } tmr_get_timesec(tstim) ; /* this is the setup time */ /* these are some abbreviations */ nl = trecParams.nl; nsamps = trecParams.nsamps; minviews = trecParams.minviews; minviewsl = minviews + 2 * nl; /* actual number of views needed */ /* tell what we know so far */ if (!quiet) { if (dorebin) { printf("tree, rebin fan:%g nviews:%d nsamps:%d rw:%d fd:%d rot:%d\n", trecParams.fanang * 180 / PI, trecParams.nviews, nsamps, trecParams.rwidth,trecParams.dofold, trecParams.rot) ; printf( "tree. mv:%d rscale:%g cf:%d c2d:%g nl:%d ecl:%g rl:%g nk:%d eck:%g\n", minviews, trecParams.rscale, trecParams.docf, trecParams.clip2d, nl, trecParams.eel, trecParams.rl, trecParams.nk, trecParams.eck) ; ) printf("tree. pviews:%d cwidth:%d fwidth:%d iwidth:%d flip:%d scale:%g\n", trecParams.pviews, trecParams.cwidth, trecParams.f idth, trecParams.iwidth, trecParams.doflip, trecParams.scale) ; if( !trecParams.cb) printf("tree. x0:%g y0:%g reconr:%g kernel:%d\n", trecParams.xO, trecParams.yO, trecParams.reconr, trecParams.ktype) ; else printf("tree. x0:%g y0:%g reconr:%g coner:%g kernel:%d\n", trecParams. O, trecParams.yO, trecParams.reconr, trecParams.coner, trecParams. type) ; printf("tree. nt:%d beta:%g nq:%d fr:%d si:%d itype:%d\n", trecParams.nt, trecParams.beta, trecParams.nq, trecParams.fr, trecParams.si, trecParams.itype) ; if(trecParams.gridr > 0) printf("tree. gridr:%d gridw:%d\n", trecParams.gridr, trecParams.gridw) ; printf("tree. Tbls:%d Mem:%d Setup time:%g\n", trecTables.memtot, trecMemory.memtot, stim) ; } /* time to ask for input file, if file cannot be opened will ask again */ getinput: tottim = 0.0; if (!infile[0]) /* file not specified on input line */ { if (noni) { printf("tree. Error, no input file εpecified.\n") ; exit(l); } printf("Enter input: ") ; getε(infile) ; ) strcpy(fname, infile); /* check to εee that file can be opened */ if (!(fp = pu_fopen(fname, "r"))) { if (noni) { printf("tree. Error opening input file %s.\n", fname); exit(l) ; } printf("tree. Cannot open file:%s\n", fname); infile[0] = 0; goto getinput; } /* read in the input data */ if (Jquiet) printf("tree. Reading input sinogram.\n") ; tmr_start_timesec() ; /* readinput gets the data. It knows whether the data is fan beam or parallel beam. */ viewsread = readinput(trecMemory.fansino, trecMemory.psino, fctrecParams, dorebin, skip, fp) ,- if (viewsread <= 0) { printf("tree. Error reading from file %s.\n", fname); if (noni) exit(l); infile[0] = 0; goto getinput; } tmr_get_timesec(&timl) ; /* keep track of file read time to give some idea of file read speed. for the MC860 in runmc mode it is very slow */ if (iquiet) printf("tree. Sino input time: %.2f \n", timl); if(!trecParams.cb) goto getout; /* in cone beam mode we need two input sinograms */ getinput2: if (!infile2[0]) { if (noni) { printf("tree. Error, no second input file εpecified.\n") ; exit(l); ) printf("Enter second input filename:"),- gets(infile2) ; ) strcpy(fname, infile2) ; if (!(fp = pu_fopen(fname, "r"))) { if (noni) { printf("tree. Error opening input file %s.\n", fname); exit(l) ; APPENDIX 1 } printf("tree. Cannot open file:%s\n", fname); infile2[0] = 0; goto getinput2; } /* read in the input data */ if (Jquiet) printf("tree. Reading second input sinogram.\n") ; tmr_start_timesec() ; err = readinput(trecMemory.fansino2, trecMemory.psino2, ttrecParams, dorebin, skip, fp) ; if(err < viewsread) viewsread = err; if (viewsread <= 0) { printf("tree. Error reading from file %s.\n", fname); if (noni) exit(l); infile[0] = 0; goto getinput2; } tmr_get_timesec(&timl) ; if (iquiet) printf("tree. Sino2 input time: %.2f \n", timl); /* before doing the recon we check that the output file can be opened. */ getout: if (!outfile[0] ) /* outfile not specified on command line */ { if (noni) { printf("tree. Error, no output file specified.\n") ; exit(l) ; } sprintf(str, "%s.tbp", infile); /* provide a default output name */ printf("Enter output file name[%s]:", str) ; gets(outfile) ; if (Jstrlen(outfile)) εtrcpy(outfile, εtr) ; ) strcpy(fname, outfile); if (!(fp = pu_fopen(fname, "w") ) ) /* check that it can be opened */ { if (noni) { printf("tree. Error opening output file %s.\n", fname); exit(l); 1 printf("tree. Cannot open file:%s\n", fname); goto reset; ) if (!quiet) {printf("tree. Input:%s Views read:%d Output:%s\n", infile, viewsread, outfile) ; if(trecParams.cb) printf("Second input:%s\n", infile2); } /* Begin the reconstruction */ tmr_start_timesec() ; if (dorebin) { /* Rebinning step: go from fan beam sinogram in fansino to a parallel beam sinogram in psino. We need 180 + fan + 2*nl views. The 2 * nl are needed for the beta to theta interpolation, nl views at the beginning and end. Since we have read in at least 180 + fan we can create any missing views from data already read in. In the case of un-corner-filled data there are phantom views at the beginning and end of the sinogram plus the empty corners. At the present we merely fill in the nl phantom views near the good views and we don't fill in any of the corners. This is not optimal and needs work. */ vO = trecParams.npviews; vl = vO + nl; for (v = vO; v < vl; v++) { fanfillin(trecMemory.fansino, v, nl, viewsread, trecParams.nviews, nsamps, trecParams.fanang) ; if(trecParams.cb) fanfillin(trecMemory.fansino2, v, nl, viewsread, trecParams.nviews, nsamps, trecParams.fanang) ; } vO = viewsread + nl - trecParams.npviews; vl = vO + nl; if(vl > minviewsl) vl = minviewsl; for (v = vO; v < vl; v++) { fanfillin(trecMemory.fansino, v, nl, viewsread, trecParams.nviews, nsamps, trecParams.fanang) ,- if(trecParams.cb) fanfillin(trecMemory.fansino2, v, nl, viewsread, trecParams.nviews, nsamps, trecParams.fanang) ; ) if (saves) { printf("Saving filled in sinogram. width:%d length:%d\n", nsamps, minviewsl); i = fwrite(trecMemory.fansino, εizeof(REAL32) , minviewsl * nsamps, fp) ; if (i != minviewsl * nsamps) printf("tree. Error writing to file:%s\n", outfile); fclose(fp) ; exit(0) ; ) /* do the rebinning */ err = trecRebin(fctrecParams, ..trecTables, ttrecMemory) ; tmr_get_timesec(&timl) ; tottim = timl; if (!quiet) printf("tree. Rebin time: %.2f \n", timl); if (err) { printf("tree. Error:%d when rebinning.\n", err) ; exit(l) ; } if (savep) { printf("Saving rebinned sinogram. width:%d length:%d\n", trecParams.rwidth, trecParams.pviews) ; i = fwrite(trecMemory.psino, εizeof(REAL32) , APPENDIX 1 trecParams.rwidth * trecParams.pviews, fp) ; if (i != trecParams.rwidth * trecParams.pviews) printf("tree. Error writing to file:%s\n", outfile); fclose(fp) ; if(trecParams.cb) { sprintf(εtr, "%s.l2", infile); printf("tree. Enter second output file name[%s] :", str); gets(outfile) ; if ( ϊstrlen(outfile) ) εtrcpy(outfile, str); strcpy(fname, outfile); if (!(fp = pu_fopen(fname, "w"))) { printf("tree. Cannot open file:%s\n", fname); exit(l); } i = fwrite(trecMemory.psino2, εizeof(REAL32) , trecParams.rwidth * trecParams.pviews, fp) ; if (i != trecParams.rwidth * trecParams.pviews) printf("tree. Error writing to file:%s\n", outfile); fclose(fp) ; } exit(O) ; } }/* if dorebin */ /* the convolved and trensformed sinos are saved from inside tbp */ if (savec) printf("tree. Saving convolved sinogram. width:%d length:%d\n", trecParams.rwidth, trecParams.pviews) ; if (savet) printf("tree. Saving tranεformed sinogram. width:%d length:%d\n", trecParams.cwidth, trecParams.pviews) ; tmr_εtart_timeεec() ; tbp(&trecMemory, ttrecTableε, fctrecParams, εaveflg, fp) ; if(εavec || εavet) /* exit in thiε case */ { fclose(fp) ; exit(O) ; } tmr_get_timesec(&tim2) ; tottim += tim2; if(!quiet) printf("tree. TBP time:%.2f\n", tim2); if (savef) { if (!quiet) printf("tree. Saving Fourier image, width:%d\n", trecParams.fwidth) ; i - fwrite(trecMemory.fimage, εizeof(REAL32) , trecParams.fwidth * (trecParams.fwidth + 2), fp) ; if (i != trecParams.f idth * (trecParams.fwidth + 2)) printf("tree. Error writing to file:%s\n", fname); fcloεe(fp); exit(O) ; } /* do the inverse 2D FFT */ tmr_start_timesec() ; /* get the Fourier image into the format required by rfft2d */ mformat(trecMemory.fimage, trecParams.fwidth, trecParams.fwidth) ; if (εavem) { if (!quiet) printf("tree. Saving M format Fourier image, width:%d\n", trecParams.fwidth) ; i = fwrite(trecMemory.fimage, εizeof(REAL32) , trecParams.fwidth * trecParams.fwidth , fp) ,- if (i != trecParams.fwidth * trecParams.fwidth) printf("tree. Error writing to file:%s\n", fname); fclose(fp) ; exit(O) ; ) /* do the 2D real inverse FFT. We need to "flip" the image */ rfft2dsh(trecMemory.fimage, trecParams.fwidth, trecParams.fwidth, 1, 1, 0); tmr_get_timesec(&tim3) ; tottim += tim3; if(ϊquiet) printf("tree. 2DFFT time: %.2f\n", tim3); if (saver) { if {!quiet) printf("tree. Saving real image, width:%d\n", trecParams.fwidth) ; i = fwrite(trecMemory.fimage, εizeof(REAL32) , trecParams.fwidth * trecParams.fwidth, fp) ; if (i != trecParams.fwidth * trecParams.fwidth) printf("tree. Error writing to file:%s\n", fname); fclose(fp) ; exit(0); } tmr_εtart_timesec() ; /* final step is to divide by the transform of the convolution function, clip and fix to an integer */ norm_iπιage(fittrecTables, &trecMemory, fctrecParams, debug | saven); tmr_get_timesec(&tim4) ; tottim += tim4; if(lquiet) printf("tree. Norm time: %.2f\n", tim.4) ; if(!quiet) printf("tree. Total time:%.2f\n", tottim); if(debug | | saven) printf(*tree. Saving real %dx%d image.\n", trecParams.iwidth, trecParams.iwidt if(debug || saven) i = fwrite(trecMemory.image, εizeof(REAL32) , trecParams.iwidth * trecParams.iwidth, fp) ; else i = fwrite(trecMemory.image, sizeof(INT16) , trecParams.iwidth * trecParams.iwidth, fp) ; if (i != trecParams.iwidth * trecParams.iwidth) { printf("tree. Error writing to file:%s\n", fname); exit(5) ; ) fclose(fp) ; if (!quiet) printf(*tree. Finished.\n") ; reset: APPENDIX 1 outfile[0] = 0; infile[0] = 0; infile2[0] = 0; if(doagain) goto getinput;/* mainly to test ability to do repeated recons */ /* 5d.) Termination Code: */ exit{0); } /* END main */ /* ♦ifdef MC860 */ EXPORT FILE * pu_fopen(strl, str2) CHAR *εtrl, *εtr2; £ return (fopen(εtrl, εtr2)); } /* ♦endif */ /* little program to initialize all the parameters we need */ INT initparams(recontype, trecParams) INT recontype; TREC_PARAMS *trecParams; { /* the default is MS100 */ trecParams->nviews = 1440; trecParams->nsamps = SMPL_PER_VTEW_100; trecParams->pviews = 720; trecParams->rwidth = 1024; trecParams->dofold = 1; trecParams->docf = 1; trecParams->doflip = 1; trecParams->nl = 3; trecParams->nk = 6; trecParams->rot = 360; trecParams->si = 0; trecParams->cb = 0; trecParams->reverse = 0; trecParams->fwidth = 1024; trecParams->cwidth = 2048; trecParams->npviews = 12; trecParams->cfslim = 520; trecParams->cfblim = 180; trecParams->fr = 512; trecParams->gridr = -1; trecParams->gridw = 0; trecParams->iwidth = 512; trecParams->nt = 5; trecParams->nq = 1024; trecParams->cutoff = -1.0; trecParams->beta = 10.3; trecParams->ktype = 0; trecParams->itype = 0; trecParams->xO = 0.0; trecParams->y0 = 0.0; trecParams->ctmin = 0.0; trecParams->ctmax = 4095.0; trecParams->ctconst = 0.0; trecParams->zout = 0; trecParams->fanang = FAN_ANGLE_100 * PI / 180. trecParams->reconr = 1.0; trecParams->coner = .5; trecParams->cbdist = .03; trecParams->rscale = 4.2296; trecParams->εcale = 1.0; trecParams->sampoffset = 0.0; trecParams->clip2d = 0.02; APPENDIX 1 trecParams->tshift = 0.0; trecParams->ecl = 1.0; trecParams->eck = 1.0; trecParams->rl = 1.15; trecParams->rk = 1.0; switch (recontype) { case MS50: trecParams->nviews = 720; trecParams->nsamps = SMPL_PER_VTEW_50; trecParams->pviews = 360; trecParams->rwidth = 512; trecParams->docf = 2; trecParams->nl = 2; trecParams->nk = 4; trecParams->rot = 180; trecParams->fwidth = 512; trecParams->cwidth = 1024; trecParams->fr = 320; trecParams->gridr = -1; trecParams->gridw = 0; trecParamε->iwidth = 256; trecParamε->fanang = FAN_ANGLE_50 * PI / 180.; trecParams->clip2d = 0.08; trecParams->npviews = 6; trecParams->cfslim = 260; trecParams->cfblim = 90; break; case TESTR1: trecParams->nviews = 512; trecParams->nsamps = 256; trecParams->pviews = 256; trecParams->rwidth = 256; trecParams->rot = 483; trecParams->dofold = 1; trecParams->docf = 0; trecParams->doflip = 0; trecParams->nl = 2; trecParams->nk = 3; trecParams->fwidth = 512; trecParams->cwidth = 512; trecParams->fr = 256; trecParams->gridr = -1; trecParams->gridw = 0; trecParams->iwidth = 256; trecParams->fanang = 42. * PI / 180.; trecParams->rscale = 1.0; trecParams->clip2d = 0.0; trecParams->npviews = 0; trecParams->cfslim = 0; trecParams->cfblim = 0; break; } return{0); ) /* * File Name: trecTbp.c * * Author : Jon Harman * Brief Description: TBP functions for tree. * * Copyright 1993 Imatron, Inc. * Command Line Synopsis: * Long Description: * Deficiencies / bugs: * * Return (statuε) codes, error messages: * Abbreviations used: * * Revision History (latest updates first!): 3/15/93 (jonh) New. */ /* LINTLIBRARY *//* suppresεes some unneeded lint messages */ /* 1.) "Imported" data types and defines: */ /* l.a.) Standard C include files */ ♦include <stdio.h> ♦include <math.h> ♦include <string.h> ♦ifndef CSPI ♦include <sys/types.h> ♦endif ♦ifdef MC860 ♦include <mcos.h> ♦include <εal_defs.h> ♦endif /* l.b.) Imatron ../include files */ ♦include "../include/imatron.h" /* first Imatron include */ /* I.e.) Project include files */ ♦include "trec.h" /* l.d.) Other include files */ /* 2.) Externals defined in this file (declarations onry): */ /* 3.) "Imported" externals: */ /* 3.a.) Imported from standard C Library */ IMPORT CHAR *malloc(); /* 3.b.) Imported from ../xxxxx */ /* 3.c.) Imported from other files in this dtrectory */ /* 3.d.) Imported.from elsewhere */ IMPORT INT debug; /* 4.) "Private" data types, defines, data and code */ ♦ifdef MC860 IMPORT REAL32 salcache[4]; ♦elεe ♦define SALJNC 1 ♦define SAL_NCC 1 ♦define SAL_CCN 1 ♦define SAL_CNC 1 ♦define SAL_CN 1 ♦define SAL_CC 1 ♦define SAL_C 1 PRIVATE REAL32 εalcache[2048] ; ♦endif PRIVATE INT ncalc = 0; PRIVATE REAL stab[NCALC] ,itab[NCALC] ; /* 5.) Exported Functions and Data: */ /* This is the main transform domain backprojection routine. It goes through the views and backprojects them using Fourier techniques (also called gridding.) My main reference for this technique is: Backprojection by Upsampled Fourier Series Expansion and Interpolated FFT in vol 1 of IEEE tranε on Image Processing. By: Makoto Tabei and Mitsuhiro Ueda */ EXPORT INT tbp(trecMemory, trecTableε, trecParams, εaveflg, fp) TREC_MEMORY *trecMemory; TREC_TABLES *trecTables; TREC_PARAMS *trecParams; INT εaveflg; /* indicated if any diagnoεtic results should be saved */ FILE *fp; /* file for εaving diagnoεtic results */ {INT i, j, k, v, pv, qv, rv, rwidth, nr, vw, cw, fr; REAL32 *psino, *psino2; REAL32 *viewl, *view2, *view3, *view4; REAL32 *cbviewl, *cbview2, *cbview3, *cbview4; REAL vangle, pvangle, qvangle, rvangle; CHAR str[100]; /* some abbreviations */ vw = trecParams->rwidth; /* view width */ cw = trecParams->cwidth; /* convolution width */ nr = trecParams->cwidth / 2; fr = trecParams->fr; psino = trecMemory->psino; pεino2 = trecMemory->pεino2; viewl = trecMemory->viewl; view2 = trecMemory->view2; view3 = trecMemory->view3; view4 - trecMemory->view4; cbviewl = trecMemory->cbviewl; cbview2 = trecMemory->cbview2; cbview3 = trecMemory->cbview3; cbview4 = trecMemory->cbview4; /* zero out the Fourier image */ init_img(trecMemory->fimage, trecParams->fwidth) ; /* v is the view variable */ for(v = 0;v < trecParams->pviews / 4; v++) { if(debug) {printf("Enter v[%d]:",v); gets(str) ,- if(strlen(str) ) v = atoi(str); } vangle = PI * (REAL) v / (REAL) trecParams->pviews; /* pv is the view at PI/2 - v */ pv = trecParams->pviews / 2 - v; if(!v) pv = trecParams->pviews / 4; /* special case */ /* qv is the view at PI/2 + v */ qv = trecParams->pviews / 2 + v; if(!v) qv = trecParams->pviews / 2; /* εpecial case */ APPENDIX 1 /* rv is the view at PI/2 + v */ rv = trecParams->pviews - v; if(!v) rv = 3 * trecParams->pviews / 4; /* special case */ if(debug) {pv = v; qv = v; rv = v;printf("vangle:%g\n",vangle*180/PI) ; } pvangle = PI * (REAL) pv / (REAL) trecParams->pviews; qvangle = PI * (REAL) qv / (REAL) trecParams->pviews; rvangle = PI * (REAL) rv / (REAL) trecParams->pviews; vclr(viewl + vw, 1, cw - vw); vclr(view2 + vw, 1, cw - vw); vclr(view3 + vw, 1, cw - vw); vclr(view4 + vw, 1, cw - vw) ,- if(trecParams->cb) { vclr(cbviewl + vw, 1, cw - vw); vclr(cbview2 + vw, 1, cw - vw) ; vclr(cbview3 + vw, 1, cw - vw); vclr(cbview4 + vw, 1, cw - vw) ; ) vmov(psino + v * vw, 1, viewl, 1, vw); vmov(psino + pv * vw, 1, view2, 1, vw); vmov(psino + qv * vw, 1, view3, 1, vw) ; vmov(psino + rv * vw, 1, view4, 1, vw) ; if(trecParams->cb) { vmov(psino2 + v * vw, 1, cbviewl, 1, vw) ; vmov(psino2 + pv * vw, 1, cbview2, 1, vw); vmov(psino2 + qv * vw, 1, cbview3, 1, vw); vmov(pεino2 + rv * vw, 1, cbview4, 1, vw) ; ) if(debug) /* only want one copy of view */ {vclr(view2, 1, cw) ; vclr(view3, 1, cw) ; vclr(view4, 1, cw); if(trecParams->cb) {vclr.(cbview2, 1, cw) ; vclr(cbview3, 1, cw) ; vclr(cbview4, 1, cw); } ) /* do the convolution by the parallel beam kernel */ kerconv(viewl, trecTables->kernel, cw) ,- kerconv(view2, trecTables->kernel, cw) ; kerconv(view3, trecTables->kernel, cw); kerconv(view4, trecTables->kernel, cw); if(trecParamε->cb) { kerconv(cbviewl, trecTables->kernel, cw) ; kerconv(cbview2, trecTables->kernel, cw) ; kerconv(cbview3, trecTables->kernel, cw) ; kerconv(cbview4, trecTables->kernel, cw) ; if (saveflg & SAVEC) /* write out convolved sino {fwrite(viewl, εizeof(REAL32) , vw, fp) fwrite(view2, εizeof(REAL32) , vw, fp) fwrite(view3, εizeof(REAL32) , vw, fp) fwrite(view , εizeof(REAL32) , vw, fp) if(trecParamε->cb) {fwrite(cbviewl, εizeof(REAL32) , vw, fp) fwrite(cbview2, εizeof(REAL32) , vw, fp) fwrite (cbview3 , sizeof (REAL32 ) , vw, fp); fwrite (cbview4 , εizeof (REAL32 ) , vw, fp); } continue; /* now circularly shift the convolved view */ cshift(viewl, vw, nr) ; cεhift(view2, vw, nr); cεhift(view3, vw, nr); cshift(view4, vw, nr) ; if(trecParams->cb) { cshift(cbviewl, vw, nr) ; cεhift(cbview2, vw, nr) ; cεhift(cbview3, vw, nr) ; cεhift(cbview4, vw, nr) ; ) /* transform */ rfft(viewl, nr, 1) rfft(view2, nr, 1) rfft(view3, nr, 1) rfft(view4, nr, 1) if(trecParams->cb) { rfft(cbviewl, nr, 1) rfft(cbview2, nr, 1) rfft(cbview3, nr, 1) rfft(cbview4, nr, 1) } /* fold around nr */ foldview(viewl, nr) ; foldview(view2, nr) ; foldview(yiew3, nr) ; foldview(view4, nr); if(trecParams->cb) { foldview(cbviewl, nr) ; foldview(cbview2, nr) ; foldview(cbview3, nr) ; ϊoldview(cbview , nr) ; } /* multiply by the interpolation filter */ vmul(viewl, 1, trecTables->ifil, 1, viewl, 1, fr * 2) vmul(view2, 1, trecTables->ifil, 1, view2, 1, fr * 2) vmul(view3, 1, trecTables->ifil, 1, view3, 1, fr * 2) vmul(view4, 1, trecTables->ifil, 1, view4, 1, fr * 2) if(trecParamε->cb) { vmul(cbviewl, 1, trecTables->ifil, 1, cbviewl, 1, fr * 2) vmul(cbview2, 1, trecTables->ifil, 1, cbview2, 1, fr * 2) vmul(cbview3, 1, trecTables->ifil, 1, cbview3, 1, fr * 2) vmul(cbview4, 1, trecTables->ifil, 1, cbview4, 1, fr * 2) } /* perform a εhift by multiplying in the Fourier domain the εhift workε on 2 (plus 2 cone beam) views at once, they must satiεfy vangle2 = PI - vanglel if(v != 0) { εhifttransv(trecTables, trecMemory, trecParams, vangle, v, viewl, view4, cbviewl, cbview4) ; APPENDIX 1 εhifttransv(trecTables, trecMemory, trecParams, pvangle, pv, view2, view3, cbview2, cbview3) ; ) else { εhifttransv(trecTables, trecMemory, trecParams, vangle, v, viewl, view3, cbviewl, cbview3) ; shifttransv(trecTables, trecMemory, trecParams, pvangle, pv, view2, view4, cbview2, cbview4) ; } /* write out transformed sino */ if (εaveflg & SAVET) {fwrite(viewl, εizeof(REAL32) , cw, fwrite(view2, sizeof(REAL32) , cw, fwrite(view3, εizeof(REAL32) , cw, fwrite(view4, εizeof(REAL32) , cw, if(trecParams->cb) {fwrite(cbviewl, sizeof(REAL32) fwrite(cbview2, εizeof(REAL32) fwrite(cbview3, sizeof(REAL32) fwrite(cbview4, sizeof(REAL32) } continue; } /* finally we do the backprojection. fbackp uses symmetry of the sines and cosines of our angles to save computation. Thus it does all four views at once. fbackpcb could do the same, but the complication is tremedous. Maybe sometime in the future. */ if( !trecParams->cb) fbackp(trecTables, trecMemory, trecParams, vangle, v) ; else { ncalc = 0; fbackpcb(trecTables, trecMemory, trecParams, vangle, viewl, cbviewl, 0); fbackpcb(trecTables, trecMemory, trecParams, pvangle, view2, cbview2, 0) fbackpcb(trecTables, trecMemory, trecParams, qvangle, view3, cbview3, 1) fbackpcb(trecTables, trecMemory, trecParams, rvangle, view4, cbview4, 1) if(ncalc > NCALC) printf("tree. Error! ! ncalc:%d v:%d\n",ncalc, v) ,- } if(debug) break; }/* for v = ... */ return(0) ; } /* fold view. This effectively doubles the frequency range of the view, and eliminates ringing artifacts. To make the higher frequencies we reflect and conjugate the view around nr in the freq domain. */ INT foldview(view, nr) REAL32 *view; INT nr; {INT i;REAL32 negl = -1.0; viewtO] *= .5; viewtnr] = view[l],-/* rfft format puts real part of nr at 1 */ vie ϊl] = 0.0; /* don't bother with this term */ viewϊnr + 1] = 0.0;/* true due to real fft symmetry */ vmov(view + nr - 2, -2, view + nr + 2, 2, nr/2 - 1) ; vsmul(view + nr - 1, -2, tnegl, view + nr + 3, 2, nr/2 - 1); /* for(i=l;i < nr/2; i++) { view[nr + i * 2] = view[(nr - i * 2)]; viewϊnr + i * 2 + 1] = -view[(nr - i * 2) + 1] ; } */ return(0) ; /* kerconv: do the convolution by transforming , multiplying, and transforming back, cw is the width of the padded view. The view must be padded to at least twice it's length to avoid errors in convolution. */ /* do the convolution with the kernel by multiplying in the Fourier domain */ INT kerconv(view, kernel, cw) REAL32 *view, *kernel; INT cw; { /* forward rfft */ rfft(view, cw, 1); /* do the convolution in freq domain by a complex multiply */ cvmul(view + 2, 2, kernel + 2, 2, view + 2, 2, (cw / 2) - 1, 1); /* these points are special due to real fft format */ view[0] *= kernel[0]; viewϊl] *= kernelϊl]; /* reverse rfft */ rfft(view, cw, -1) ; return(0) ; ) /* circularly shift the convolved view by 180 degrees */ INT cεhift(view, vw, nr) REAL32 *view; INT vw, nr; { /* εave the first half */ vmov(view, 1, view + nr, 1, vw / 2); /* move second half to firεt half */ vmov(view + vw / 2, 1, view, 1, vw / 2); /* move saved first half to second half */ vmov(view + nr, 1, view + nr - vw / 2, 1, vw / 2); if(nr > vw) vclr(view + vw / 2, 1, nr - vw); return(0) ; ) Transform domain backprojection routine. This routine backprojects four views at once. One is at vangle, the others at PI/2-vangle, PI/2 + vangle. PI-vangle. APPENDIX 1 This allows us to save a little calculation by making use of the symmetries of sines and cosines. The first view (viewO = 0) is a special case. The backprojection is done in the transform domain by convolving the view with an nt x nt convolving function then adding into the 2D Fourier matrix. For each complex point in the view we need to calculate the coordinates (kx0,ky0) in the big matrix of the little nt x nt matrix. We also calculate the coefficients of the little matrix. Since it is separable, we need two nt length vectors: vx and vy. These use valueε precalculated and saved in the grtable. INT fbackp(trecTables, trecMemory, trecParams, vangle, viewO) TREC_TABLES *trecTables; TREC_MEMORY *trecMemory; TREC_PARAMS *trecParamε; REAL vangle; INT viewO; {INT i, fr; REAL rεin, rcoε; REAL32 *grtable; INT32 *vkxO = trecMemory->vkxO,*vkyO = trecMemory->vkyO; REAL32 **wx = trecMemory->w , "wy = trecMemory->wy; REAL32 *vs = trecMemory->vs; REAL32 *viewl, *view2, *view3, *view4; viewl = trecMemory->viewl; /* the view at vangle: (rcoε, -rεin) */ view2 = trecMemory->view2; /* the view at PI/2 - vangle: (rsin, -rcos) */ view3 = trecMemory->view3; /* the view at PI/2 + vangle: (-rsin, -rcos) */ view4 = trecMemory->view ; / the view at PI - vangle: (-rcos, -rsin) */ if(trecParams->doflip && (viewO != 0)) {/* flip causes first coord to get negated */ viewl = trecMemory->view4; /* the view at PI - vangle: (rcos, -rsin) */ view2 = trecMemory->view3; /* the view at PI/2 + vangle: (rsin, -rcos)*/ view3 = trecMemory->view2; /* the view at PI/2 - vangle: (-rsin, -rcos) */ view4 = trecMemory->viewl; /* the view at vangle: (-rcos, -rsin)*/ /* fr is the length (in coπrplex elements) of the view that we backproject */ fr = trecParams->fr; grtable = trecTables->grtable; if(view0 != 0) { rcos = trecParams->reconr * 2, 0 * cos(vangle) ; rsin = trecParams->reconr * 2, 0 * sin(vangle) ; /* calculate the matrix coords and the coefficientε for -rcoε and -rεin */ calccoord(trecParamε, grtable, 0.0, -rcos, vkxO, wx, vs) ,- calccoord(trecParamε, grtable, 0.0, -rεin, vkyO, wy, vε); /* now do the gridding into the matrix */ /* view4 is at (-rcos, -rsin) */ vgrid(trecParams, trecMemory, trecTables, vkxO, vkyO, wx, wy, view4) ; /* view3 is at (-rsin, -rcos) */ vgrid(trecParams, trecMemory, trecTableε, vkyO, vkxO, wy, wx, view3); /* view2 iε at (rsin, -rcos) */ /* have to calculate rsin, stash results in view3 and view4 */ calccoord(trecParams, grtable, 0.0, rsin, view3, view4, vs) ; vgrid(trecParams, trecMemory, trecTables, view3, vkxO, view4, wx, view2); /* viewl is at (rcos, -rsin) */ /* have to calculate rcos, staεh reεults in view3 and view4 */ calccoord(trecParams, grtable, 0.0, rcos, view3, view4, vs); vgrid(trecParams, trecMemory, trecTables, view3, vkyO, view4, wy, viewl); } APPENDIX 1 else { /* view 0 is a special case, here we store vangle = 0 in viewl at (1,0) flip: (-1,0) vangle = PI/4 in view2 at (.707,-.707) flip: (-.707,-.707) vangle = PI/2 in view3 at (0,-1) flip: (0,-1) vangle = 3PI/2 in view4 at (-.707,-.707) flip: (.707,-.707) if(!trecParams->doflip) { rcos = trecParams->reconr * 2.0; rsin = 0.0; calccoord(trecParams, grtable, 0.0, rcos, vkxO, wx, vε) ; calccoord(trecParams, grtable, 0.0, rsin, vkyO, wy, vs) ; vgrid(trecParams, trecMemory, trecTables, vkxO, vkyO, wx, wy, viewl) ; calccoord(trecParams, grtable, 0.0, -rcos , vkxO, wx, vs) ; vgrid(trecParams, trecMemory, trecTables, vkyO, vkxO, wy, wx, view3) ; rcos = trecParams->reconr * 2.0 * cos(PI / 4.0) rεin = trecParams->reconr * 2.0 * sin(PI / 4.0) calccoord(trecParamε, grtable, 0.0, rcos, vkxO, wx, vs); calccoord(trecParams, grtable, 0.0, -rsin vkyO , wy, vs) ; vgrid(trecParams, trecMemory, trecTables, vkxO, vky0, wx, wy, view2) ; vgrid(trecParams, trecMemory, trecTables, vkyO, vkyO, wy, wy, view4) ; ) else { rcos = -trecParams->reconr * 2 0; rsin = 0.0; calccoord(trecParams, grtable, calccoord(trecParams, grtable, vgrid(trecParams, trecMemory, vgrid(trecParams, trecMemory, rcos = trecParams->reconr * 2. rsin = trecParams->reconr * 2. calccoord(trecParams, grtable, calccoord(trecParams, grtable, vgrid(trecParams, trecMemory, vgrid(trecParams, trecMemory, } return(0) ,- ) /* Transform domain cone beam backprojection routine. This routine backprojects two views (the cone beam pair at vangle) at once. The goal of the cone beam algorithm is to weight each view with a linear weighting function during backprojection. It does this by convolving the view with a simple weight function in the Fourier domain. In fact we use a sine function near the zero croεεing, but very much zoomed in, to approximate a linear weighting function in the εpatial domain. Thiε requires a convolution by a two point function. One point is at (sx0,sy0) with complex value cmull.re,cmull.im. The other iε at (-εx0,-sy0) and has complex value cmull.re, -cmull.im. The second view has the same vangle but is shaded oppositely, i.e. the shading direction is the same, but the weighing function haε opposite εlope. We εave time by uεing the same vspread routine to do both views: we just add the two views before vspread. */ INT fbackpcb(trecTableε, trecMemory, trecParams, vangle, viewl, view2, opp) TREC_TABLES *trecTables; TREC_MEMORY *trecMemory; TREC_PARAMS *trecParams; REAL vangle; REAL32 *viewl, *view2; APPENDIX 1 INT opp; {INT i, fr, cindex, cwidth = trecParams->cwidth; REAL sxO, εyO, rεin, rcos, cbdist, cbmult, val, va2, tsh, cbscale; INT32 *vkx0 ,*vkyO; REAL32 " x, vvy; REAL32 *cbtempl = trecMemory->cbtempl, *cbtemp2 = trecMemory->cbtemp2; COMPLEX32 cmull, cmul2; fr = trecParams->fr; /* the parameters that govern the cone beam shading are: cbscale: a scale factor that reflects the deεired slope of the shade function. For reconr = 1 and coner = 1 the shade function will go from 0 to 1 over iwidth (center half of fimage) . This corresponds to a cbscale of 1. For reconr = .5, coner = 1.0 we want the shade function to go from .25 to .75 so cbscale = .5. cbdiεt: diεtance from 0 of each cb term. If cbdist - 1 then the shade function will be a sine wave with period equal to fwidth (=2 * iwidth) . A smaller cbdist will result in a larger period. We want the shading function to be approximately linear so we choose a very small cbdist (.03) to begin with. (nq limits the smallness of cbdiεt) We use cbdist to implement cbscale: zooming in on the sine wave results in a lower slope for the shading function, cbmult: This is a εcale factor. It is used to establish the basic scale for reconr = coner = 1. Then cbdist is used to further scale the εhading function. tsh: An angular shift to get the sine wave into the right position. For xO = 0 and yO = 0 this means put the zero crossing of the εhading at the center of the image. In general the zero crossing must be adjusted to reflect the position of the center of the recon circle in the image. cbεcale = trecParams->reconr / trecParams->coner; cbdist = trecParams->cbdist * cbscale; cbmult = .5 / sin(trecParams->cbdist * PI / 2.0); val = vangle + PI; /* shading angle for view 1 */ va2 = vangle; /* shading angle for view 1 *1 if(opp) /* opp means shade oppositely: true for second half of views */ {val = vangle; va2 = vangle + PI; ) if(trecParams->doflip) {val = -val;va2 = -va2;} /* (rcoε,rsin) iε the angle the view iε backprojected at. It iε the εa e aε the non cone beam caεe */ rcoε = trecParams->reconr * 2.0 * cos(vangle) ; if(trecParamε->doflip) rcoε = -rcos; rsin = -trecParams->reconr * 2.0 * εin(vangle) ; /* (εxO.εyO) iε a vector offεet from the nominal position (0,0) of the backprojection. */ sxO = sin(val) * cbdist; εyO = cos(val) * cbdist; tsh = trecParams->cbdist * PI / 2.0 * (1.0 + (sin(val) * trecParams->x0 + cos(val) * trecParams->y0) * cbscale); cmull.re = cbmult * εin(tεh); cmull.im = -cbmult * cos(tsh); APPENDIX 1 if(debug) printf("vangle:%g rcos:%g rsin:%g val:%g sxO:%g syO:%g\n", vangle * 180 / PI, rcos, rsin, val * 180 / PI, sxO, syO) ; if(debug) printf("cbdiεt:%g tεh:%g cml.re:%g cml.im:%g\n", cbdist, tsh * 180 / PI, cmull.re, cmull.im); cbcc(trecParams, trecTables, trecMemory, sxO, rcos, fccindex) ; vkxO = (INT32 *) trecMemory->cbcoords + cindex * cwidth; wx = (REAL32 **) vkxO + cwidth / 2; cbcc(trecParams, trecTables, trecMemory, syO, rsin, &cindex) ; vkyO = (INT32 *) trecMemory->cbcoords + cindex * cwidth; wy = (REAL32 **) vkyO + cwidth / 2; tεh = trecParams->cbdist * PI / 2.0 * (1.0 + (εin(va2) * trecParams->x0 + cos(va2) * trecParamε->yO) * cbscale); cmul2.re = cbmult * εin(tεh); cmul2.im = cbmult * coε(tεh); /* note the difference */ if(debug) printf("cml: %g %g cm2:%g %g\n",cmull.re,cmull.im, cmul2.re,cmul2.im) ; /* multiply the views by their complex coefficients */ cvcsml(viewl, 2, &cmull, cbtempl, 2, fr) ; cvcsml(view2, 2, &cmul2, cbtemp2, 2, fr) ; /* add the two views */ vadd(cbtempl, 1, cbtemp2, 1, cbtempl, 1, 2 * fr) ,- vgrid(trecParams, trecMemory, trecTables, vkxO, vkyO, wx, wy, cbtempl); sxO = -sin(val) * cbdist; syO = -cos(val) * cbdist; cbcc(trecParams, trecTables, trecMemory, sxO, rcoε, tcindex) ; vkxO = (INT32 *) trecMemory->cbcoords + cindex * cwidth; wx = (REAL32 **) vkxO + cwidth / 2; cbcc(trecParams, trecTables, trecMemory, εyO, rεin, fccindex) ,- vkyO = (INT32 *) trecMemory->cbcoords + cindex * cwidth; wy = (REAL32 **) vkyO + cwidth / 2; /* for the second backprojection the coefficients are conjugated */ cmull.im = -cmull.im; cmul2.im = -cmul2.im; /* multiply by the coefficients */ cvcsml(viewl, 2, tcmull, cbtempl, 2, fr) ; cvcsml(view2, 2, &cmul2, cbtemp2, 2, fr) ; /* add the two views */ vadd(cbtempl, 1, cbteπrp2, 1, cbtempl, 1, 2 * fr) ; vgrid(trecParams, trecMemory, trecTableε, vkxO, vkyO, wx, wy, cbtempl); retur (0) ; ) /* Cone beam coordinate calculation. We backproject 4 views at once because due to symmetry we can get away with half the coordinate calculations. For non-cone beam we actually figured out the εymmetries for the 4 backprojections. For cone beam there are 8 backprojectionε and 16 coordinate calcs. This is just too many different cases to consider. Therefore we try a different approach. The coordinate calculation depends on sO and inc. We store the pairs (sO.inc) and coordiante arrays that we have already calculated. Then APPENDIX 1 for each new coordinate calc we check if (sO,inc) match a previously calculated pair. If so we use the previous pair's array, if not we calculate a new one. */ ♦define ACCUR (5.0e-9) INT cbcc(trecParams, trecTables, trecMemory, sO, inc, cindex) TREC_PARAMS *trecParams; TREC_TABLES *trecTables; TREC_MEMORY *trecMemory; REAL sO, inc; INT *cindex; { INT i, cwidth = trecParams->cwidth; INT32 *vk; REAL32 **w; /* look to see if we have already calculated these coords */ for(i=0;i<ncalc;i++) {if((fabs(εO - εtab[i]) < ACCUR) && (fabs(inc - itab[i]) < ACCUR)) {*cindex = i; return(0) ; } } /* need to calculate a new set */ vk = (INT32 *) trecMemory->cbcoords + ncalc * cwidth; w = (REAL32 **) vk + cwidth/2; calccoord(trecParams, trecTables->grtable, sO, inc, vk, w, trecMemory->vs) ; stab[ncalc] = sO; itab[ncalc] = inc; *cindex = ncalc++; return(0) ; } /* calccoord creates a vector of real coordinates: vs[i] = sO + inc * i. For each of those coordinates it chooses an integer position vkO, for the start of the convolution function (width nt) and an error term d that representε the diεtance from the center of the function to v[i] Thiε error term is then converted into an addresε w[i] , that pointε to the correct entry in grtable for that error. */ INT calccoord(trecParams, grtable, sO, inc, vkO, w, vε) TREC_PARAMS *trecParams; REAL32 *grtable; REAL sO, inc; /* offset and increment for the coordinates */ INT32 *vkO; /* output array of integer coordinates */ REAL32 **w; /* output array of addresεeε */ REAL32 *vε; /* a temp εtorage array */ { INT32 nt2, nt4, nfml, ntodd, nr, fr, ibignum, beg, nr2, r; INT32 casize = 2048; REAL32 nquantr, rsO, rinc, rnt5, rbignum, zero = 0.0, one = 1.0; REAL32 *ca = salcache; rinc = inc; /* ditto */ nquantr = trecParams->nq; /* ditto */ nt2 = trecParams->nt / 2; nt4 = trecParamε->nt * 4; nfml = trecParams->fwidth - 1; ntodd = ( (nt2 * 2) != trecParams->nt) ; nr = trecParams->cwidth / 2; fr = trecParams->fr; rεO = sO; /* need a REAL32 */ APPE 1 /* for nt odd we sub .5 to get error between 0 and 1 instead of -.5 to .5 */ if(ntodd) rsO -= .5; rnt5 = trecParams->nt * .5; if(ntodd) rnt5 -= .5; rbignum = -3 * nr - rnt5; ibignum = 3 * nr; /* create a vector of coordinateε. our object is to translate this into a εet of integers plus real fractionε. The fractions are converted into addresses into the grtable */ ♦if 0 /* this way isn't faster than the optimized makecoord */ /* just in case fr might get larger than casize we stripmine the data */ for(beg = 0; beg < fr;beg += casize) {nr2 = fr - beg; if(nr2 > casize) nr2 = casize; /* the stuff with bignum calcs ceil(vs[i] - nt5) */ rεO = εO + beg * rinc; if(ntodd) rsO -= .5; vrampx( rsO, trine, ca, 1, nr2,SAL_C); vmovx(ca, 1, vs, 1, nr2, SAL_CN) ; vεaddx(ca, 1, trbignum, ca, 1, nr2,SAL_CC) ; vfix32x(ca, 1, ca, 1, nr2, SAL_CC) ; vεaddix(ca, 1, tibignum, ca, 1, nr2, SAL_CC) ; vmovx(ca, 1, vkO + beg, 1, nr2, SAL_CN) ; /* now we must calculate the error d = (vkO[i] + nt/2) - vs[i]*/ vsaddix(ca, 1, tnt2, ca, 1, nr2, SAL_CC) ; vflt32x(ca, 1, ca, 1, nr2, SAL_CC) ; vsubx(vs, 1, ca, 1, ca, 1, nr2, SAL_NCC) ; /* need thiε for nq = 4096 && clOO */ vclipx(ca, 1, zero, tone, ca, 1, nr2, SAL_CC) ; /* have calculated the fractions and made εure they are between 0 and 1 */ /* now convert into an addreεs */ vsmulx(ca, 1, tnquantr, ca, 1, nr2, SAL_CC) ; vfix32x(ca, 1, ca, 1, nr2, SAL_CC) ; vεmulix(ca, 1, fcnt4, ca, 1, nr2, SAL_CC) ; vεaddix(ca, 1, tgrtable, w + beg, 1, nr2, SAL_CN) ,- } /* finally we make εure the integerε are in the range 0 .. nfml */ for(r = 0; r < fr; r++) vk0[r] &= nfml; ♦endif makecoord(trsO, trine, vkO, w, trecParams->nt, trbignum, tnquantr, ibignum, nfml, grtable, fr) ; retur (0) ; } /* routine to calc the coordinates. This was done by ESAL routines, but we now have an assemble lang routine to do it. This explains why it has been split off from calccoordε */ ♦ifdef UNIX int makecoord(arεO, arinc, vkO, w, nt, arbignum, anquantr, ibignum, nfml, grtable, fr) REAL32 *ars0, *arinc; INT32 *vk0; REAL32 **w; REAL32 *arbignum, *anquantr; INT nt, ibignum, nfml, fr; APPENDIX 1 REAL32 *grtable; {INT i, nt4, nt2, itmp; REAL32 rtmpl, rtmp2, rbignum, nquantr, rsO, rinc; nt2 = nt / 2; rbignum = *arbignum; nquantr = *anquantr; rsO = *arsO; rinc = *arinc; rtmpl = rεO; for(i=0;i<fr;i++) {rtmp2 - rtmpl + rbignum; itmp = rtmp2; itmp += ibignum; *vkO++ = itmp t nfml; itmp += nt2; rtmp2 = itmp - rtmpl; if(rtmp2 > 1.0) rtmp2 = 1.0; if(rtmp2 < 0) rtπrp2 - 0.0; rtmp2 *= nquantr; itmp = rtmp2; itmp *= nt; *w++ = itmp + grtable; rtmpl += rinc; } } ♦endif /* vgrid:perform gridding of input vector into the Fourier image */ /* Input iε: vectors of length nr: vkx0,vxy0, wx,wy,q also gw, * a 2D inverse FFT. * Output is gw. * vkx0,vky0 hold the x and y matrix positionε for each point * wx,wy hold pointerε to the x and y gridding function array. * q holds the complex point to be gridded. * * From paper: Backprojection by Upsampled Fourier Series Expansion * and Interpolated FFT * By: Makoto Tabei and Mitsuhiro Ueda * For each point in q we are given the coords (kxO.kyO) of the beginning * point in the matrix for the nt x nt rectangle. We also have the * horizontal (vx) and vertical (vy) arrays of the separable gridding * function. The array gw is actually of width mx/2 complexes and * length my + 2 rows. The last two rows hold the column at freq mx/2. * For each r from 0 to nr-1 we multiply the complex number q[r] * by a ntxnt matrix of coefficients wx[r] [j] * wy[r] [k] , * where j,k go from 0 to nt-1 and add the ntxnt values into gw * starting at vkxO[r] ,vky0[r] . * I have never tested this with mx != my. */ EXPORT INT vgrid(trecParams, trecMemory, trecTables, vkxO, vkyO, wx, wy, q) TREC_PARAMS *trecParamε; TREC_MEMORY *trecMemory; TREC_TABLES *trecTableε; INT *vkxO, *vky0; REAL32 **wx, "wy; COMPLEX32 *q; {INT jx, jy, kx, ky, ky_f, kxO, kyO, r; INT mx, my, nt, nr, w; REAL32 v_re, v_im, vy_re , CL re , q_im, *vx, *vy; INT mxd2; COMPLEX32 *gw, *gwl, *qt; nr = trecParamε->fr; nt - trecParamε->nt; APPE IX 1 mx ■ = trecParams->fwidth; my = mx; gw = (COMPLEX32 *)trecMemory->fimage; /* a εcheme for increasing speed: use smaller nt for higher frequencies */ /* only working for nt = 5 */ if( (trecParams->gridr > 1) tt (nt == 5)) {qt = (COMPLEX32 *)trecMemory->gridtmp; r = trecParams->gridr; w = trecParams->gridw; if(w == 200) return(O);/* secret test code */ /* grid the low frequencies */ vgrid5(gw, mx, my, nt, r - w, vkxO, vkyO, wx, wy, q) ; /* grid the high frequencies */ vgrid3x(gw, mx, my, nt, nr - r - w, vkxO + r + w, vkyO + r + w, wx + r + w, wy + r + w, q + r + w) ; if(w == 0) return(O); /* feather the intermediate frequencies */ vmuKq + r - w, 1, trecTableε->feather, 1, qt, 1, 4 * w) ; /* grid the intermediate frequencies */ vgrid5(gw, mx, my, nt, 2 * w, vkxO + r - w, vkyO + r - w, wx + r - w, wy + r - w, qt) ; /* feather the low end of the high */ vεub(qt, 1, q + r - w, 1, qt, 1, 4 * w) ; /* do the high freq gridding */ vgrid3x(gw, mx, my, nt, 2 * w, vkxO + r - w, vkyO + r - w, wx + r - w, wy + r - w, qt) ; return(0) ; } /* for the caεes nt = 4, 5, 7 we use specifically tailored routines to maximize speed */ if(nt == 5) {vgrid5(gw, mx, my, nt, nr, vkxO, vkyO, wx, wy, q) ; return(0) ; ) else if(nt == 4) {vgrid4(gw, mx, my, nt, nr, vkxO, vkyO, wx, wy, q) ; return(0) ; > else if(nt == 7) {vgrid7(gw, mx, my, nt, nr, vkxO, vkyO, wx, wy, q) ,- retur (0) ; } /* compute some conεtantε. */ mxd2 = mx / 2; for(r=0; r<nr; r++) { kxO « *vkx0++; kyO = *vky0++; vx = *wx++; vy = *wy++; /* Map 2-D convolution of q onto gw on gw */ q_re = q[r] .re; q_im = q[r] .im; APPENDIX 1 if((kxO + nt) <= mxd2) { ky = kyO; for(jy = 0; jy < nt; jy++) { v_re = q_re * vy[jy] ; v_im = q_im * vyϊjy] ; kx = kxO; gwl = gw + mxd2 * ky; for(jx = 0;jx < nt; jx++) { gwl[kx].re += v_re * vx[jx]; gwl[kx].im += v_im * vxϊjx]; kx++; ) if((++ky) == my) ky = 0; } continue; } if((kxO > mxd2) &t (kxO <= mx - nt)) { if(kyO == 0) ky_f = 0; elεe ky_f = my - kyO; for(jy = 0; jy < nt; jy++) { v_re = q_re * vy[jy] • v_im = q_im * vyϊjy]; kx = mx - kxO; gwl = gw + mxd2 * ky_f; for(jx = 0;jx < nt; jx++) { gwl[kx].re += v_re * vx[jx]; gwl[kx).im -= v_im * vx[jx],- —; ) if((~ky_f) < 0) ky_f = my - 1; } continue; } /* εeparating out the above εpecial cases speeds up the algorithm, the following code can handle all caseε, but is slower so we uεe it for what iε left over from the above. */ kx = kxO; for(jx = 0; jx < nt; jx++) { v_re = q_re * vx[jx]; v_im = q_im * vx[jx] ; if(kx <= mxd2) /* check folding */ { ky = kyO; if(kx != mxd2) { gwl = gw + kx; for(jy - 0; jy < nt; jy++) { gwl[mxd2 * ky] .re += v_re * vy[jy] ; gwl[mxd2 * ky] .im += v_im * vy[jy] ; if((++ky) == my) ky = 0; ) ) /* note the special encoding, the kx = mx/2 column is stored in the last two rows */ else { gwl = gw + mxd2 * my; for(jy = 0; jy < nt; jy++) APPENDIX 1 { gwl [ky] .re += v_re * vy[jy] ,- gwl [ky] . im += v_im * vyϊjy] ,- if ( (++ky) == my) ky = 0 ; } ) } else { if ( kyO == 0) ky_f = 0; else ky_f = my - kyO ; gwl = gw + (mx - kx) ; for (jy = 0; jy < nt; jy++) { gwl[mxd2 * ky_f] .re += v_re * vytjy] ; gwl[mxd2 * ky_f] .im -= v_im * vyϊjy); if((~ky_f) < 0) ky_f = my - 1; ) } if((++kx) == mx) kx = 0; } } return(0) ; ) /* vgrid */ ♦ifdef UNIX /* for 860 use assembly lang version */ /* vgrid:perform gridding of input vector into the Fourier image */ /* Input is: vectors of length nr: vkx0,vxy0, wx,wy,q also gw, a 2D inverse FFT of width mx (i.e. mx/2 complexes) and height my For our case mx always equals my. Output is gw. gw has two extra rows holding the high freq terms of the other rows vkxO.vkyO hold the x and y matrix positions for each point wx.wy hold pointers to the x and y gridding function array, q holdε the complex point to be gridded. For each r from 0 to nr-1 we multiply the complex number q[r] by a ntxnt matrix of coefficients wx[r] [j] * wy[r] [k] , where j,k go from 0 to nt-1 and add the ntxnt values into gw starting at vkxO[r] ,vky0[r] . */ /* εpecial version for nt = 5 */ INT vgrid5(gw, mx, my, nt, nr, vkxO, vkyO, wx, wy, q) INT mx, my, nt, nr, *vkx0, *vky0; REAL32 **wx, "wy; ' COMPLEX32 *gw, *q; {INT jx, jy, kx, ky, ky_f, kxO, kyO, r; REAL32 v_re, v_im, vy_re, q_re, q_im, *vx, *vy; REAL32 vO, vl, v2, v3, v4; INT mxd2; COMPLEX32 *gwl; /* compute some conεtantε. */ mxd2 = mx / 2; f* main loop */ for(r=0; r<nr; r++) { /* get the position in the matrix */ kxO = *vkx0++; kyO = *vky0++; /* get the addreεε of the gridding fcnε */ vx - *wx++; vy = *wy++; /* get the input complex points */ q_re = q[r] .re; APPENDIX 1 q_im = q[r) . im; /* get the x gridding coefficients */ /* divide the work into 3 εpecial cases depending on kxO */ /* first is case 1: kxO + 4 < mx/2 */ if((kxO + 5) <= mxd2) { ky = kyO; for(jy = 0; jy < 5; jy++) { v_re = q_re * vy[jy] ; v_im = q_im * vyϊjy] ; kx = kxO; gwl = gw + mxd2 * ky; gwl[kx].re += v_re * vO; gwlϊkxj.im += v_im * vO; kx++; gwl[kx].re += v_re * vl; gwlϊkxj.im += v_im * vl; kx++; gwl[kx].re += v_re * v2; gwl[kx] .im += v_im * v2; kx++; gwl[kx].re += v_re * v3; gwlϊkxj.im += v_im * v3; kx++; gwl[kx].re += v_re * v4; gwlϊkxj.im += v_im * v4; if((++ky) == my) ky = 0; } continue; ) /* second is case 2: kxO > rox/2 and kxO <= mx - 5 */ if((kx0 > mxd2) tt (kxO <= mx - 5)) { if(ky0 == 0) ky_f = 0; elεe ky_f = my - kyO; for(jy = 0; jy < 5; jy++) { v_re = q_re * vy[jy] ; v_im = q_im * vyϊjy] ; kx = mx - kxO; gwl = gw + mxd2 * ky_f; gwl[kx].re += v_re * vO; gwlϊkxj.im -= v_im * vO; kx—; gwl[kx].re += v_re * vl; gwlϊkxj.im -= v_im * vl; x—; gwl[kx].re += v_re * v2; gwlϊkx].im -= v_im * v2; —; gwl[kx].re += v_re * v3; gwlϊkxj.im -= v_im * v3; kx—; gwl[kx].re += v_re * v4; gwlϊkxj.im -= v_im * v4; if((~ky_f) < 0) ky_f = my - 1; ) continue; } /* separating out the above special cases speeds up the algorithm, the following code can handle all cases, but is slower so we ' uεe it for what is left over from the above. */ kx = kxO; for(jx = 0; jx < 5; jx++) { v_re = q_re * vxljx]; v_im = q_im * vx[jx]; if(kx <= mxd2) /* check folding */ { ky = kyO; if(kx != mxd2) /* this is the kx < mx/2 case */ { gwl = gw + kx; for(jy = 0; jy < 5; jy++) { gwl[mxd2 * ky] .re += v_re * vy[jy] ; gwlΪmxd2 * ky] .im += v_im * vyϊjy] ; if((++ky) == my) ky = 0; > } /* note the εpecial encoding, the kx = mx/2 column is stored in the last two rows */ else /* this is the kx = mx/2 case */ { gwl = gw + mxd2 * my; for(jy = 0; jy < 5; jy++) { gwl[ky].re += v_re * vy[jy] ; gwlϊky] .im += v_im * vyϊjy] ,- if((++ky) == my) ky = 0; } ) ) else /* this is the kx > mx/2 case */ { if( kyO == 0) ky_f = 0; elεe ky_f = my - kyO; gwl = gw + (mx - kx) ; for(jy = 0; jy < 5; jy++) { gwl[mxd2 * ky_f] .re += v_re * vy[jy] ; gwlΪmxd2 * ky_f] .im -= v_im * vyϊjy] ; if((—ky_f) < 0) ky_f = my - 1; } ) if((++kx) == mx) kx = 0; ) ) return(O) ; } /* vgridδ */ ♦endif /* spread out the convolution functionε into the Fourier image */ /* εpecial verεion for nt = 4 */ EXPORT INT vgrid4(gw, mx, my, nt, nr, vkxO, vkyO, wx, wy, q) INT mx, my, nt, nr, *vkx0, *vky0; REAL32 **wx, "wy; COMPLEX32 *gw, *q; {INT jx, jy, kx, ky, ky_f, kxO, kyO, r; REAL32 v_re, v_im, vy_re, q_re, q_im, *vx, *vy; REAL32 vO, vl, v2, v3; INT mxd2; APPENDIX 1 COMPLEX32 *gwl; /* compute εome conεtants. */ mxd2 = mx / 2; for(r=0; r<nr; r++) { kxO = *vkxO++; kyO = *vkyO++; vx = *wx++; vy = *wy++; /* Map convolution function on gw */ q_re = q[r] .re; q_im = q[r] .im; if((kxO + 4) <= mxd2) { ky = kyO; for(jy = 0; jy < 4; jy++) { v_re = q_re * vy[jy] ; v_im = q_im * vyϊjy] ; kx = kxO; v3; if((++ky) == πty) ky = 0; } continue ,- } if((kx0 > mxd2) && (kxO <= mx - 4)) { if(ky0 == 0) ky_f = 0; elεe ky_f = τw - kyO; for(jy = 0; jy < 4; jy++) { v_re = q_re * vy[jy]; v_im = q_im * vyϊjy]; kx = mx - kxO; gwl = gw + mxd2 * ky_f ; gwl[kx].re += v_re * vO; gwlϊkxj.im -= v_im * vO; — ; gwl[kx].re += v_re * vl; gwlfkxj.im -= v_im * vl; k — ; gwl[kx].re += v_re * v2; gwlϊkxj.im -= v_im * v2; k — ; gwl[kx].re += v_re * v3; gwlϊkxj.im -= v_im * v3; if{(— ky_f) < 0) ky_f = my - 1; APPENDIX 1 } continue ; } ,- ; mx/2 column is stored in the else { gwl = gw + mxd2 * my; for(jy = 0; jy < 4; jy++) { gwl[ky].re += v_re * vy[jy); gwlϊkyϊ.im += v_im * vyϊjy]; if((++ky) == my) ky = 0; ) ) } else { if{ kyO == 0) ky_f = 0; elεe ky_f = my - kyO; gwl = gw + (mx - kx) ; for(jy = 0; jy < 4; jy++) { gwl[mxd2 * ky_f] .re += v_re * vy[jy] ; gwlΪmxd2 * ky_f].im -= v_im * vyϊjy] ; if((~ky_f) < 0) ky_f = my - 1; ) } if((++kx) == mx) kx = 0; } ) return(0) ; } /* vgrid4 */ /* spread out the convolution functionε into the Fourier image */ /* εpecial verεion for nt = 7 */ EXPORT INT vgrid7(gw, mx, my, nt, nr, vkxO, vkyO, wx, wy, q) INT mx, my, nt, nr, *vkx0, *vky0; REAL32 "wx, "wy; COMPLEX32 *gw, *q; {INT jx, jy, kx, ky, ky_f, kxO, kyO, r; REAL32 v_re, v_im, vy_re, q_re, q_im, *vx, *vy; REAL32 vO, vl, v2, v3, v4, v5, v6; INT mxd2; COMPLEX32 *gwl; /* compute some constants. */ mxd2 = mx / 2; APPENDIX 1 for(r=0; r<nr; r++) { kxO = *vkxO++; kyO = *vkyO++; vx = *wx++; vy = *wy++; /* Map 2-D convolution function on gw */ q_re = q[r] .re; q_im = q[r] .im; if((kxO + 7) <= mxd2) { ky = kyO; for(jy = 0; jy < 7; jy++) { if((++ky) == my) ky = 0; } continue } if((kx0 > mxd2) tt (kxO <= mx - 7)) { if(ky0 == 0) ky_f = 0; elεe ky_f = my - kyO; for(jy = 0; jy < 7; jy++) { v_re = q_re * vy[jy] ; v_im = q_im * vyϊjy] ; kx = mx - kxO; gwl = gw + mxd2 * ky_f; gwl[kx].re += v_re * vO; gwlϊkxj.im -= v_im * vO; kx--; gwl[kx].re += v_re * vl; gwlϊkx].im -= v_im * vl; gwl[kx].re += v_re * v5; gwlϊkxj.im -= v_im * v5; kx — ; gwl[kx].re += v_re * v6; gwlϊkxj.im -= v_im * v6; if({— ky_f) < 0) ky_f = my - 1; } continue; ) kx = kxO; for(jx = 0; jx < 7; jx++) { v_re = q_re * vx[jx]; v_im = q_im * vxϊjx]; if (kx <= mxd2) /* check folding */ { ky = kyO; if (kx != mxd2) { gwl = gw + kx; for(jy = 0; jy < 7; jy++) { gwl[mxd2 * ky] .re += v_re * vy[jy] ; gwl[mxd2 * ky] .im += v_im * vyϊjy]; if((++ky) == my) ky = 0; ) } /* note the εpecial encoding, the kx = mx/2 column iε εtored in the laεt two rows */ else { gwl = gw + mxd2 * my; for(jy = 0; jy < 7; jy++) { gwl[ky].re += v_re * vy[jy] ,- gwlϊkyj.im += v_im * vyϊjy] ; if((++ky) == my) ky = 0; } ) ) else { if( kyO == 0) ky_f = 0; else ky_f = my - kyO; gwl = gw + (mx - kx) ; for(jy = 0; jy < 7; jy++) { gwl[mxd2 * ky_f] .re += v_re * vy[jy] ; gwlΪmxd2 * ky_f] .im -= v_im * vyϊjy] ; if((—ky_f) < 0) ky_f = my - 1; } } if((++kx) s= mx) kx = 0; ) retur ( 0 ) ; APPENDIX 1 } /* vgrid7 */ ♦ifdef UNIX INT vgrid3x(gw, mx, my, nt, nr, vkxO, vkyO, wx, wy, q) INT mx, my nt, nr, *vkxO, *vkyO; REAL32 **wx, "wy; COMPLEX32 *gw, *q; {INT jx, jy, kx, ky, ky_f, kxO, kyO, r; REAL32 v_re, v_im, vy_re, q_re, q_im, *vx, *vy; REAL32 vO, vl, v2, v3, v4; INT mxd2; COMPLEX32 *gwl; /* compute some constantε. */ mxd2 = mx / 2; for(r=0; r<nr; r++) { kxO = *vkxO++; kyO = *vkyO++; vx = *wx++; vy = *wy++; /* Map 2-D convolution function on gw */ q_re = q[r] .re; σ_im = q[r] . im; vl = vx[l]; v2 = vxΪ2) ; v3 = vx ϊ 3 ] ; if((kxO + 5) <= mxd2) /* i.e. kxO + 4 < mx/2 */ { ky = kyO; if((++ky) == my) ky = 0; i - 5)) - 1; for(jy = 1; jy < 4; jy++) { v_re = q_re * vy[jy] ; v_im = q_im * vyϊjy] ; gwl = gw + mxd2 * ky_f ,- kx = mx - kxO - 1; gwl [ kx] .re += v_re * vl; APPENDIX 1 if((— y_f) < 0) ky_f = my - 1; } continue; ) /* separating out the above special cases speeds up the algorithm, the following code can handle all cases, but is slower so we use it for what is left over from the above. */ case */ /2 column is εtored in the } return(0) ; APPENDIX 1 } /* vgrid3x */ ♦endif * ** ** * * * * ** * *** ** ** * * v.nr of trecTbp.c *** **** ** * * * ** * * * * ** **/ /* * File Name: trecTable.c * * Author : Jon Harman * Brief Description: Creates tables for tree. * * Copyright 1993 Imatron, Inc. * * Command Line Synopsis: * * Long Description: * Deficiencies / bugs: * * Return (status) codes, error messages: * Abbreviations used: * * Revision History (latest updates first!): 3/10/93(jonh) New. */ /* LINTLIBRARY *//* suppresses some unneeded lint mesεages */ /* 1.) "Imported" data types and defines: */ /* l.a.) Standard C include files */ ♦include <stdio.h> ♦include <math.h> /* l.b.) Imatron ../include files */ ♦include " ../include/imatron.h" /* first Imatron include */ /* I.e.) Project include files */ ♦include "trec.h" /* l.d.) Other include fileε */ /* 2.) Externals defined in thiε file (declarationε only): */ FORWARD INT trecRBTable() ; /* 3.) "Imported" externals: */ /* 3.a.) Imported from standard C Library */ /* 3.b.) Imported from ../xxxxx */ /* 3.c.) Imported from other files in this dtrectory */ /* 3.d.) Imported from elsewhere */ PRIVATE INT debug = 0; /* 4.) "Private" data types, defines, data and code */ /* for debugging purposes */ PRIVATE INT isd = -1, iεgd = -1; PRIVATE REAL tεinc() , gridfen() ; /* 5.) Exported Functions and Data: */ /* * rebinning table creation routine, the tables created are nnsigma, "* nnbeta, phi, psi. memory iε allocated for them, total memory used is * added to memtot */ EXPORT INT trecRBTable(trecParams, trecTables) TREC_PARAMS *trecParams; /* parameters that define the rebinning */ TREC_TABLES *trecTables; /* pointers to memory for tables */ { REAL soffset = -.5, r = 1000.0; APPENDIX 1 REAL betaO, dbeta, thetaO, dtheta, sigmaO, dεigma, εO, ds; REAL sig a, beta, bmin, bmax, accum, accumk; REAL ang, rnk, ml; INT32 nbeta, ntheta, nεigma, nε, nphi; INT32 ibeta, itheta, iεigma, is, ithetaO; ΪNT32 i, k, 1, 11, iang, betaflag, maxb, minb, minviews; INT32 nnl, nnk; UINT16 *nnsigma, *nnbeta; REAL32 *phi, *psi; CHAR str[100]; /* * Allocate the nearest neighbor tables. These give the closest fan * geometry point to a given parallel geometry point. */ nnεigma = (UINT16 *) malloc(trecParams->rwidth * εizeof(*nnεigma) ) ; nnbeta = (UINT16 *) malloc(trecParams->nsampε * εizeof(*nnbeta) ) ,- if (!nnbeta || Jnnεigma) { printf("trecTable: Cannot get memory for nn tables\n"); return (-1) ; } /* * Allocate the phi and psi tables. These are the main interpolation * tables, psi[iε,iεigma] phi[isigma,ibeta] . */ phi = (REAL32 *) malloc(trecParams->nεamps * trecParams->nl * 2 * εizeof(REAL32) ) ; pεi = (REAL32 *) malloc(trecParamε->rwidth * trecParamε->nk * 2 * εizeof(REAL32) ) ; if ( !psi I I !phi) { printf("trecTable: Cannot get memory for psi,phi tables\n"); return (-2) ,- } /* update memory usage */ trecTables->memtot += trecParams->rwidth * εizeof(*nnεigma) + trecParams->nεamps * sizeof(*nnbeta) + (trecParams->nsamps * trecParams->nl * 2 + trecParams->rwidth * trecParams->nk * 2) * εizeof(REAL32) ,- trecTableε->nnεigma = nnεigma; trecTables->nnbeta = nnbeta; trecTables->phi = phi; trecTables->psi = pεi; if (debug) { iεd = 100; isgd = 100; /* printf("Enter isd[%d] isgd[%d]:", iεd, iεgd) ; gets(str) ,- if (εtrlen(εtr) > 0) sεcanf(str, "%d %d", tisd, tisgd) ; */ } /* first we determine the limits for our variables */ /* beta is the fan geometry view number */ betaO = 0.0; dbeta = PI / trecParams->pviews; nbeta = trecParams->pviews * 2; trecParams->minviews = (trecParams->fanang + PI) * trecParams->pviewε / PI + .5; nnl = 2 * trecParams->nl; nnk = 2 * trecParams->nk; rnl = (REAL) trecParams->nl; rnk = (REAL) trecParams->nk; /* sigma iε the fan geometry εample position, equal angle samples. */ dsigma = trecParams->fanang / (trecParams->nsamps - 1) ; εigmaO = (-trecParams->fanang / 2.0) + trecParams->εampoffεet * dsigma; nsigma = trecParamε->nsamps; /* theta iε the parallel geometry view number */ ntheta = nbeta / 2; dtheta = dbeta; /* dtheta must = dbeta to use the phi table */ thetaO = betaO + dbeta * trecParams->nl + (nsigma - 1) * dsigma + sigmaO; ithetaO = thetaO / dtheta + .5; itheta0++; /* a little extra */ thetaO = ithetaO * dtheta; /* we want thetaO to be a power of dtheta */ thetaO += trecParams->tεhift; /* ε iε the parallel geometry εample poεition */ dε = 2 * r * εin(trecParams->fanang / 2.0) / (trecParams->rwidth - 1) ; εO = r * sin(-trecParams->fanang / 2.0) + εoffset * ds; ns = trecParams->rwidth; /* * Create the nearest neighbor tables. These give the closest fan * geometry point to a given parallel geometry point. */ bmin = TWOPI; bmax = 0.0; for (is = 0; is < ns; is++) { εigma = aεin((is * ds + sO) / r) ,- i = (εigma - εigmaO) / dεigma - trecParams->nk + 1.0; if (i < 0) i = 0; if (i > nsigma - nnk) i = nsigma - nnk; if (is == isd) printf("is:%d εigma:%g nnεigma:%d\n", iε, εigma, i) ; nnsigma[is] = i; ) minb = trecParams->minviews; maxb = 0; for (isigma = 0; isigma < nsigma; isigma++) { εigma = isigma * dsigma + sigmaO; beta = thetaO - εigma; if (beta < bmin) bmin = beta; if (beta > bmax) bmax = beta; ibeta = (beta - betaO) / dbeta - trecParams->nl + 1.0; if (isigma == isgd) printf("iεg:%d εigma:%g beta:%g nnbeta:%d\n", isigma, εigma, beta, ibeta) ,- if(ibeta < minb) minb = ibeta; if(ibeta > maxb) maxb = ibeta; nnbeta[isigma] = ibeta; } if(maxb - minb + ntheta > trecParams->minviews) trecParams->minviews = maxb - minb + ntheta; if (debug) printf("rbtable: Finished with nn tables. min:%d max:%d\n",minb, maxb); APPENDIX 1 /* * Create the phi and pεi tables. These are the main interpolation * tables. psi[iε,k] phi[1,isigma] . */ if (debug) printf("rbtable: Making psi and phi Tables.\n"); /* * make the phi table. This is used for the initial (beta, εigma) to * (theta, sigma) interpolation */ for (isigma = 0; iεigma < nsigma; isigma++) { accum = 0.0; for (1 = 0; 1 < nnl; 1++) { sigma = isigma * dsigma + sigmaO; beta = (nnbeta[isigma] + 1) * dbeta + betaO; ang = beta + εigma - thetaO; if (ang > PI) ang = ang - TWOPI; if (ang < -PI) ang = ang + TWOPI; ang = ang / dbeta; accumk = tsinc(ang * trecParams->rl, rnl, trecParams->ecl) ,- /* * if(nnl > 2) accumk = tsinc(ang * trecParams->rl, rnl, * trecParams->ecl) ; else { if(ang > 0) accumk = 1.0 - ang; else * accumk = 1.0 + ang; } */ phi[l + iεigma * nnl) = accumk; accum += accumk; if (iεigma == iεgd) printf("isg:%d l:%d sigma:%g beta:%g ang:%g phi:%g accum:%g\n", iεigma, 1, εigma, beta, ang, phi[l * nεigma + iεigma], accum); } if (accum > 0.0) for (1 = 0; 1 < nnl; 1++) phi[l + iεigma * nnl] /= accum; } /* adjust nnbeta to start at 0 */ for (isigma = 0; isigma < nεigma; iεigma++) nnbeta[iεigma] -= minb; /* * make the pεi table. Thiε iε uεed in the (theta,εigma) to (theta,ε) * interpolation */ for (is = 0; iε < nε; iε++) { accum = 0.0; for (k s 0; k < nnk; k++) { sigma = (nnεigma[iε] + k) * dεigma + εigmaO; ang = aεin((iε * dε + εO) / r) - εigma; if (ang > PI) ang = ang - TWOPI; if (ang < -PI) ang = ang + TWOPI; ang = ang / dεigma; accumk = tεinc(ang * trecParamε->rk, rnk, trecParams->eck) ,- accum += accumk; psi[k * ns + is] = accumk; if (is == isd) printf("iε:%d k:%d εigma:%g ang:%g psi:%g accum:%g\n", is, k, εigma, ang, pεi[k * ns + is], accum); if (accum > 0.0) for (k = 0; k < nnk; k++) psi[k * ns + iε] /= accum; ) if (debug) printf("\n") ; if (debug) printf("rbtable: Finiεhed with pεi and phi tables.\n"); return (0) ; } /* * truncated, tapered sine interpolation for rebinning. x iε the point at * which we evaluate the interp function, n is the order of the * interpolation (i.e. uses 2n points), it is used to scale the gausεian * taper, larger n leεε taper, k iε alεo used to scale the taper, larger k * more taper. I have also used k to allow for linear interp or for * 4 point interpolation using Wallschlaeger's algorithm. If k iε negative * then Wallεchlaeger's algorithm is used with w = -k -1. */ PRIVATE REAL tsinc(x, n, k) REAL x, k, n; { REAL xn; if (x < 0.0) x = -x; if (x == 0.0) return 1.0; xn = x / n; if(k >= 0) return (sin(x * PI) / (x * PI) ) * exp(-x * xn * k) ; else /* try Wallschlager's interpolation function */ {if(x > 2.0) return(0.0); if(x > 1.0) return((-k - 1.0) * (.5 * x - 1.0)); return(-k + (1.5 * k + .5) * x) ; ) } /* make the conεtant data needed for TBP routines. This includes: FFT weights: used by Mercury in fft routines convolution kernel: parallel beam Laks kernel. Others can be input interpolation filter: filter for folded transformed view table for convolution function spatial domain transform of convolution function. Used to norm image. ramp for shift rans */ EXPORT INT trecTBPTable(trecParams, trecTables) TREC_PARAMS *trecParams; /* parameters that define the rebinning */ TREC_TABLES *trecTables; /* pointers to memory for tables */ { INT i, j, k, kw, fr, tsize; CHAR kerfile[100] ; /* εtring εpecifying a kernel file */ FILE *fpε; REAL32 rtempi, rtemp2; REAL beta2; /* AP fft routineε need weights table */ ♦ifndef CSPI kw = MAX(trecParams->cwidth, trecParams->fwidth) ,- trecTableε->weightε = (REAL32 *) malloc(kw * sizeof(REAL32) * 2); if ( !trecTables->weightε) { printf("tree: Cannot get memory for weights array.\n") ,- return(-1) ; ) trecTables->memtot += kw * sizeof(REAL32) * 2; /* initialize */ fftwtε(trecTables->weights,kw,kw) ; ♦endif /* next get memory and initialize the convolution kernel */ trecTableε->kernel = (REAL32 *) malloc(trecParams->cwidth * sizeof(REAL32) ) ; if (!trecTables->kernel) { printf("tree: Cannot get memory for kernel.\n"); return(-1) ; } trecTables->memtot += trecParams->cwidth * sizeof(REAL32) ; if(trecParams->ktype <= -1) { printf("Enter kernel file name:"); gets(kerfile) ; fps = fopen(kerfile, "r"); if (!fps) { printf("Unable to open kernel file %s.\n", kerfile) ; trecParams->ktype = 0; } elεe { i = fread(trecTables->kernel, sizeof(REAL32) , trecParams->cwidth, fps); if(i != trecParams->cwidth) { printf("Kernel file too small! cwidth:%d size:%d\n", trecParams->cwidth, i); trecParams->ktype = 0; ) fclose(fpε) ,- ) * } if(trecParams->ktype >= 0) makekernel(trecParams->cwidth, trecParams->ktype, trecParamε->cutoff, trecTableε->kernel) ; /* next get memory and initialize the interpolation filter */ trecTables->ifil = (REAL32 *) malloc(trecParams->cwidth * sizeof(REAL32) ) ; if (!trecTableε->ifil) { printf("tree: Cannot get memory for interpolation filter.\n"); return(-1) ; } trecTableε->memtot += trecParamε->cwidth * εizeof(REAL32) ; for{i=0;i<trecParamε->cwidth;i++)trecTableε->ifil[i] = 0.0; fr = trecParams->fr; if( !trecParams->si) fr = trecParams->cwidth / 2; make_ifil(fr, trecParams->itype, trecTables->ifil, trecParams->gridr, trecParams->gridw) ; /* juεt for debugging */ if(trecParams->itype > 5) trecParams->gridr = -1; APPE D X 1 /* make the table of Kaiser bessel values for the transform domain convolution function */ tsize = trecParams->nq * trecParams->nt; if(trecParams->gridr > 0) {tsize += trecParams->gridw * 4; } trecTables->grtable = (REAL32 *) malloc(tsize * εizeof(REAL32) ) ; if (!trecTableε->grtable) { printf("tree: Cannot get memory for kb table.\n") ; return(-1) ; } trecTables->memtot += tsize * sizeof(REAL32) ; if(trecParams->gridr > 0) trecTables->feather = trecTables->grtable + trecParams->nq * trecParams->nt; elεe trecParams->gridw = -1; make_grtable(trecParams->nt, trecParams->beta, trecTables->grtable, trecParams->nq, trecParamε->gridw) ; /* make the table of values for the spatial domain transform of the gridding function. */ trecTables->imgwin = (REAL32 *) malloc(trecParams->fwidth * sizeof(REAL32) ) ; if (!trecTables->imgwin) { printf("tree: Cannot get memory for transform kb table.\n"),• return(-1) ; } trecTables->memtot += trecParams->fwidth * εizeof(REAL32) ; make_imgwin(trecParam , trecTables->imgwin) ; /* make a ramp for shift routine */ trecTables->ramp = (REAL32 *) malloc(trecParams->cwidth * sizeof(REAL32) ) ; if (!trecTables->ramp) { printf("tree: Cannot get memory for ramp.\n"); return{-1) ; ) trecTables->memtot += trecParams->cwidth * sizeof(REAL32) ; rtempl = 0.0; rtemp2 = 1.0; vramp( rtempl, trtemp2, trecTables->ramp, 2, trecParams->cwidth / 2); rteπrp2 = -1.0; vramp(trtempl, trtemp2, trecTables->ramp + 1, 2,trecParams->cwidth / 2); return(0) ; } /* makekernel: make the Imatron kernels, ktype determines the kernel type 0: a straight laks kernel 1: the Imatron normal kernel:Butterworth 830, .93 1020, .00028", 2: reserved (currently straight laks) 3: head l:w .01633 .3266 .9 times Blackmann 650 1024 4: head 2:w .02768 .3266 .8305 times Blackmann 650 1024 5: head εmooth:w .01633 .3266 .9 times Hamming 500 1024 €: sharp:diff of G .5,3 1,-1 7: very sharp:3 pt -1,3 8: smooth:Hanning 0 1024 APP 9: special:3 pt -2,5 then scaled by .5 */ INT makekernel(cwidth, ktype, cutoff, kernel) INT cwidth, ktype; REAL cutoff; REAL32 *kernel; { INT i, start, εtop; REAL t,tt; /* firεt make a εtraight laks kernel with cutoff */ for (i = 0; i < cwidth; i++) { kernel[i] = 0.0; } /* set up the kernel: do it in spatial domain then transform it */ • /* parallel geometry */ tt = 1.0; kernel[0] = .25 * tt; for (i = 1; i < cwidth/2; i += 2) { t = -tt / (i * i * PI * PI) ; kernel[i] = t; kernelϊcwidth - i] = t; ) /* transform into freq domain */ rfft(kernel, cwidth, 1) ; /* add a filter */ if (cutoff > 0.0) { for (i = 0; i < cwidth/2; i++) { t = i / ((cwidth/2) * cutoff); tt = exp(-.5 * t * t); kernel[i*2] *= tt; kernel[i * 2 + 1] *= tt; } kernel[1] *= exp(-.5 / (cutoff * cutoff)),- } /* next make the special filters */ swit h(ktype) { case 0: default: break; case 1: /* normal use cutoff of 1.5,i=0 to approximate noise in fbp version */ start = (830 * cwidth) / 2048; stop = (1020 * cwidth) / 2048; butter(kernel, cwidth, start, .93, stop, .00028); break; case 2: break; case 3: walterman(kernel, cwidth, .01633, .3266, .9); start = (650 * cwidth) / 2048; stop = (1024 * cwidth) / 2048; black(kernel, cwidth, start, εtop) ,- break; case 4 : APPENDIX 1 walterman(kernel, cwidth, .02768, .3266, .8305); εtart = (650 * cwidth) / 2048; εtop = (1024 * cwidth) / 2048; black(kernel, cwidth, start, εtop); break; case 5: walterman(kernel, cwidth, .01633, .3266, .9); εtart = (500 * cwidth) / 2048; εtop = (1024 * cwidth) / 2048; hamm(kernel, cwidth, start, εtop) ; break; caεe 6: dog(kernel, cwidth, .5, 3.0, 1.0, -1.0); break; caεe 7: threept(kernel, cwidth, -1.0, 3.0); break; caεe 8: start = (0 * cwidth) / 2048; εtop = (1024 * cwidth) / 2048; harm(kernel, cwidth, εtart, εtop); break; case 9: threept(kernel, cwidth, -2.0, 5.0); for(i=0;i<cwidth;i++) kernel[i] *= .5; break; } return(0) ; ) /* make the interpolation filter. We have various types possible. Type 0 is close to linear interpolation Type 1 is intermediate Type 2 is close to cubic interpolation. Type 3 is a Gausεian, εmoother than linear Type 4 is constant at 1.0 Type 5 is sharper than cubic */ INT make_ifil(fr, itype, ifil, cutpt, delta) INT fr, itype, cutpt, delta; REAL32 *ifil; { INT i; /* create the interpolation filter fr gives the number of complex elements in the filter*/ ifil[0] = 1.0; ifil[l] = 1.0; if(cutpt == -1) cutpt = 512; if(delta <= 0) delta = 20; if(itype > 5) printf("*** εpecial test mode cut:%d delta:%d\n",cutpt, delta); if((itype == 7) || (itype == 9)) { ifil[0] = 0.0; ifilll] = 0.0; } for(i = 1; i < fr;i++) { switch(itype) { case 0:/* linear interp */ default: ifil[2 * i] = sin(PI * i / (REAL) fr) / (PI * i / (REAL) fr) ; ifil[2 * i] *= ifil[2 * i] ; brea ; caεe 1:/* a little bit εharper */ ifil[2 * i] = .5 * (1.0 + coε(PI * i / (REALMfr))); break; caεe 1 : 1* equivalent of cubic interp */ ifil[2 * i] = (8.0 + 9 * cos(PI * i / (REAL) (fr)) - cos(3.0 * PI * i / (REAL)(fr))) / 16.0; break; caεe 3: ifil[2 * i] = exp(-2 * PI * (REAL) i * i / ((REAL)fr * fr) ) ; break; caεe 4: ifil[2 * i] = 1.0; break; caεe 5: ifil[2 * i] = εqrtd.O / (1.0 + pow(2.0 * i / (REAL)fr,8.0) )) ; break; case 6: ifil[2 * i] = sin(PI * i / (REAL) fr) / (PI * i / (REAL) fr) ; ifil[2 * i] *= ifil[2 * i] ; if(i > cutpt + delta) ifil[2 * i] = 0.0; elεe if(i > cutpt - delta) ifil[2 * i] *= .5 - .5 * εin((i - cutpt) * PI / (2.0 * delta)); break; caεe 7: ifil[2 * i] = εin(PI * i / (REAL) fr) / (PI * i / (REAL) fr) ; ifil[2 * i] *= ifil[2 * i] ,- if(i <= cutpt - delta) ifil[2 * ij = 0.0; elεe if(i <= cutpt + delta) ifil[2 * i] *= .5 + .5 * εin((i - cutpt) * PI / (2.0 * delta)); break; caεe 8: ifil[2 * i] = (8.0 + 9 * cos(PI * i / (REAL) (fr) ) - cos(3.0 * PI * i / (REALMfr))) / 16.0; if(i > cutpt + delta) ifil[2 * i] = 0.0; elεe if(i > cutpt - delta) ifil[2 * i] *= .5 - .5 * εin((i - cutpt) * PI / (2.0 * delta)); break; caεe 9: ifil[2 * i] = (8.0 + 9 * cos(PI * i / (REALMfr)) - cos(3.0 * PI * i / (REALMfr))) / 16.0; if(i <= cutpt - delta) ifil[2 * i] = 0.0; elεe if(i <= cutpt + delta) ifil[2 * i] *= .5 + .5 * sin((i - cutpt) * PI / (2.0 * delta)),- break; ) ifil[2 * i + 1] = ifil[2 * i] ; } return(0) ; } /* modified Bessel function 10(x) . from Numerical Recipies in C */ REAL besseliO(x) REAL x; { REAL ax, ans, y; if((ax = fabs(x)) < 3.75) {y = ■ x / 3.75; y *= y; ans = 1 .0 + y * ( 3 .5156229 + y * ( 3 .0899424 + y * ( 1.2067492 + y * ( 0.2659732 + y * ( 0.360768e-l + y * 0.45813e-2 ) ) ) ) ) ,- } elεe { APPENDIX 1 / sgrt(ax)) * (0.39894228 + y * (0.1328592e-l .225319e-2 + y * (-0.157565e-2 + y * (0.916281e-2 0.2057706e-l + y * (0.2635537e-l + y * (-0.1647633e-l 392377e-2) ))))))); /* make the table of ID gridding functions for quantized dx's . 10(beta * εqrt(l - (2 * (u + dx) / nt)**2) / nt where -nt/2 <= u <= nt/2 (nt odd) */ EXPORT INT make_grtable( nt, beta, table, nquant, gridw) REAL beta; INT nt, nquant, gridw; REAL32 *table; { REAL u, dx; REAL32 *vx; INT jx, nq; /* table contains nt entries for each quantizied fraction nq */ for(nq = 0; nq < nquant; nq++) { vx = table + nq * nt; if(((nt / 2) * 2) == nt) /* 0 <= dx < 1., nt: even. */ dx = (nq + .5) / (REAL) nquant; else /* -.5 <= dx < .5, nt: odd. */ dx = -.5 + (nq + .5) / (REAL) nquant; /* Generate gridding function for thiε fraction */ for(jx = 0; jx < nt; jx++) { u = jx - nt/2 + dx; vx[jx] = gridfcn(beta, nt, u) ; } ) if(debug) for(jx = 0; jx < nt;jx++) printf("k:%d grtable:%g\n", jx,table[jx] ) ; if(gridw <= 0) return(O); /* create the feathering table for transition between low md high freq */ vx = table + nquant * nt; for(jx = 0; jx < gridw * 2; jx++) { vx[2 * jx] = .5 - .5 * εin((jx - gridw) * PI / (2.0 * gridw)); vx[2 * jx + 1] = vx[2 * jx] ; } return(0) ; ) /* make the transformed grid function used to normalize the image */ INT make_imgwin(trecParams, imgwin) APPENDIX 1 TREC_PARAMS *trecParams; REAL32 *imgwin; { INT i, jx; REAL u, scale; REAL32 *line; for(jx = 0; jx < trecParams->fwidth; jx++) imgwin[jx] = 0.0; for(jx = 0; jx <= trecParams->nt/2; jx++) { u = jx; imgwin[jx * 2] = gridfcn(trecParams->beta, trecParams->nt, u) ; if(debug) printf("jx:%d imgwin:%g\n",jx, imgwin[jx * 2] ) ; ) rfftsh(imgwin, trecParams->fwidth, 1, 1, 1) ; if(debug) printf("imgwin:fw/2:%g 3*fw/4:%g fw-l:%g\n", imgwin[trecParams->f idth / 2], imgwinϊ3 * trecParams->fwidth 7 4], imgwinϊtrecParams->f idth - 1]); if(debug) { line = (REAL32 *) malloc (trecParams->fwidth * 8); for(jx = 0; jx < trecParams->fwidth * 2; jx++) line[jx] = 0.0; for(jx = 0; jx <= trecParams->nt; jx++) { u = jx / 2.0; line[jx * 2] = gridfen(trecParams->beta, trecParams->nt, u) ; ) rfftshdine, trecParams->fwidth * 2, 1, 1, 1); printf("line:fw:%g 5fw/4:%g 3fw/2:%g 7fw/4:%g 2fw-l:%g\n", line[trecParams->fwidth] , lineϊδ * trecParams->fwidth / 4], lineΪ3 * trecParaιns->fwidth / 2] , lineΪ7 * trecParams->fwidth / 4], lineΪ2 * trecParams->fwidth - 1] ) ; free(line) ; εcale = trecParams->scale * .9932 * PI * PI / ( (REAL)trecParams->pviews * trecParams-S-cwidth) ; if(trecParams->cb) εcale *= .5; εcale = sqrt(εcale) ,- for{i=0;i<trecParams->fwidth;i++) if(imgwin[i] != 0.0) imgwin[i] = scale / (imgwi [i] * trecParams->f idth) ; return(0) ; } /* the gridding function in the transform domain */ PRIVATE REAL gridfen(beta, nt, u) REAL beta; INT nt; REAL u; { REAL usqr, besseliO(),- usqr = u * u * 4.0 / (nt * nt) ; return (besseliO(beta * sqrtd.O - usqr)) / besseliO(beta) ) ; APPENDIX 1 /* usqr = TWOPI * u / nt; return(.42323 + .49755 * cos( usqr) + .07922 * cos(2 * usqr)); */ ) /* kernel building routines. These implement various filters which are multiplied times the kernel */ /* butter: a Butterworth filter */ PRIVATE INT butter(kernel, cwidth, ip, pval, iε, sval) REAL32 *kernel; INT cwidth, ip, is; REAL pval,sval; { REAL el, e2, e4, order, fm, filter; INT i; el = sqrtd.O/pval - 1.0); e2 = el * el; e4 = e2 * e2; order = log(((1.0 / (sval * sval)) - 1.0)/(e4 + 2.0 * e2)) / log( (REAL)is/(REAL)ip) ; fm = (REAL) ip / pow(el * sgrt(2.0 + e2),2.0 / order); ford = 0; i < cwidth / 2,-i++) { filter = 1.0 / (sqrtd.O + pow((REAL)i / fm, order))); kernel[2 * i] *= filter; if(i > 0) kernel[2 * i + 1] *= filter; } kernel[1] *= filter; /* use last value for kernel[1] */ return(0) ; } /* Blackman filter */ PRIVATE INT black(kernel, cwidth, εtart, εtop) REAL32 *kernel; INT cwidth, εtart, εtop; { INT i, nw; REAL filter; nw = εtop - εtart; for(i = 0; i < cwidth / 2;i++) { if(i < εtart) filter = 1.0; elεe if(i > εtop) filter = 0.0; else filter = .42 - .5 * cos(PI * (i - start) / nw + PI) + .08 * cos(2.0 * (PI * (i - εtart) / nw + PI)),- kernel[2 * i] *= filter; ifd > 0) kernel[2 * i + 1] *= filter; } kernel[1] *= filter; return ( 0 ) ; ) APPENDIX 1 /* Hanning filter */ PRIVATE INT hann(kernel, cwidth, εtart, εtop) REAL32 *kernel; INT cwidth, εtart, εtop; { INT i, nw; REAL filter; nw = stop - start; for(i = 0; i < cwidth / 2;i++) { if(i < start) filter = 1.0; elεe if(i > εtop) filter = 0.0; elεe filter = .5 * (1.0 - cos(PI * (i - start) / nw + PI)); kernel[2 * i] *= filter; if(i > 0) kernel[2 * i + 1] *= filter; } kernel[1] *= filter; return(0) ; } /* Hamming filter */ PRIVATE INT hamm(kernel, cwidth, start, εtop) REAL32 *kernel; INT cwidth, εtart, εtop; { INT i, nw; REAL filter; nw = stop - εtart; ford = 0; i < cwidth / 2;i++) { if(i < εtart) filter = 1.0; else if(i > stop) filter = 0.0; elεe filter = .54 - .46 * coε(PI * (i - εtart) / nw + PI); kernel[2 * i] *= filter; ifd > 0) kernel[2 * i + 1] *= filter; ) kernel[1] *= filter; retur (0) ; } /* Difference of Gaussians filter */ PRIVATE INT dog(kernel, cwidth, εigmal, εcalel, sigma2, scale2) REAL32 *kernel; INT cwidth; REAL εigmal, scalel, εigma2, εcale2; { INT i; REAL32 filter[2048]; REAL gaussO, x; for (i = 0; i < cwidth; i++) { x = cwidth / 2 - i; filter[i] = εcalel * gauss(x, βigroal) + scale2 * gauss(x, sigma2) } APPENDIX 1 rfftsh(filter, cwidth, 0, 1); /* * some ad hoc corrections until I take the time to understand what is * going on */ x = 1.0 / filter[2]; for (i = 0; i < cwidth; i ++) { filter[i] *= x; } filtertO] = 1.0; for (i = 0; i < cwidth; i ++) { kernel[i] *= filter[i]; } retur (0) ; ) /* Three point filter */ PRIVATE INT threept(kernel, cwidth, cl, c2) REAL32 *kernel; INT cwidth; REAL cl, c2; { INT i; REAL32 filter[2048] ; REAL x; for (i = 0; i < cwidth; i++) { filter[i] = 0.0; ) filter[cwidth / 2 - 1] = cl; filter[cwidth / 2] = c2; filter[cwidth / 2 + 1] = cl; rfftsh(filter, cwidth, 0, 1); /* * some ad hoc corrections until I take the time to understand what is * going on */ filtertO] = 1.0; x = filter[2] ; filter[1] /= x; for (i = 2; i < cwidth; i += 2) { filter[i] /= x; filterd + 1] = filterd]; } for(i=0;i<cwidth;i++) kernel[i] *= filterd],- return(0) ; 5 /* Walterman head kernel:cl * exp(-c2|x|) + c3 * delta(x) */ PRIVATE INT walterman(kernel, cwidth, cl, c2, c3) REAL32 *kernel ; INT cwidth; REAL cl , c2 , c3 ; APPENDIX 1 { INT i; REAL32 filter[2048] ; REAL x; for (i = 0; i < cwidth; i++) { x = cwidth / 2 - i; if(x < 0.0) x = -x; filterd] = cl * exp(-c2 * x) ; ) filter[cwidth/2] += c3; rfftsh(filter, cwidth, 0, 1); /* * some ad hoc corrections until I take the time to understand what is * going on */ /* the head kernel is set up as a deconvolution */ filtertO) = 1.0; x = filter[2] ; filter[1] = x / filterd]; for (i = 2; i < cwidth; i += 2) { filterti) = x / filterd]; filterd + 1] = filterd]; ) for(i=0;i<cwidth;i++) kernelϋ] *= filterd); return(0) ; ) PRIVATE REAL gauss(x, sigma) REAL x, sigma; { x = x / εigma; return exp(-(x * x / 2.0)); ) /********************* Bπfl of trecTable.c **********************/ APPENDIX 1 /* * trec.h Definitions for tree * * ===> tree: Imatron TBP Reconstruction * * Revision History(latest updates first!): * 3/12/93(jonh) New. */ ♦define PI 3.141592654 ♦define TWOPI 6.283185307 ♦define TESTRl 3 /* code to indicate an alternate recon (test geometry) */ ♦define SAVEC 1 /* bit position of savec bit in saveflg */ ♦define SAVET 2 /* bit position of εavet bit in εaveflg */ ♦define NCALC 8 /* size of ncalc for cone beam */ typedef struct { float re; float im; ) COMPLEX32; /* this structure holds all the parameters that govern the reconstruction process from rebinning through final image */ typedef struct TRECPARAMS { number of views over 360 degrees */ number of samples per view */ number of views in parallel sinogram after rebinning */ /* min number of fan beam views (calc by RBtable) */ width of the rebinned parallel sinogram */ number of views to rotate */ whether to fold or not */ whether to do corner-filling or not */ whether to flip or not */ smooth interpolation filter if fr < 1 */ do cone beam recon */ order of theta interpolations in rebinning */ order of ε interpolations in rebinning */ true if rotation is reverse */ width (and height) of the Fourier image */ size (in R32'ε) of the convolution kernel */ width (and height) of the output image */ size of tbp convolution */ εize of grid table */ length of interpolation filter (in complex elements)*/ radius of transition from first to second gridding fen */ half width of transition from first to second gridding fen */ type of convolution kernel */ type of interpolation kernel */ zero out image outside of recon circle */ number of phantom views */ corner fill const */ corner fill const */ fan angle in radians */ recon radius 0 to 1 */ cone radius */ cone beam distance */ rebinning scale factor */ tbp εcale factor */ cutoff for εmoothing filter */ /* offset of samples wrt center of fan (usually 0) */ clip2d parameter in rebinning */ shift for thetaO in rebinning */ beta for tbp gridding function */ const for theta interps in rebinning */ const for s interps in rebinning */ reach for theta interps in rebinning */ APPENDIX 1 REAL rk; /* reach for ε interps in rebinning */ REAL xO; /* position of center of image (-1 to 1) */ REAL yO; /* position of center of image (-1 to 1) */ REAL32 ctmin; /* minimum CT number (0) */ REAL32 ctmax; /* max CT number (4095) */ REAL32 ctconst; /* const added to ct numbers a la Siemens */ } TREC_PARAMS; /* this structure holds all the memory pointers for tables */ typedef struct TRECTABLES { UINT32 memtot; /* total memory used in tables */ REAL32 *phi; /* phi table for rebinning */ REAL32 *psi; /* psi table for rebinning */ UINT16 *nnsigma; /* nnsigma table for rebinning */ UINT16 *nnbeta; /* nnbeta table for rebinning */ REAL32 *kernel; /* kernel */ REAL32 *ifil; /* bp interp filter */ REAL32 *weights; /* weights for FFT's */ REAL32 *grtable; /* table of gridding values */ REAL32 *feather; /* feathering for transition between gridding fens */ REAL32 *imgwin; /* transformed grid fen for normalization of image */ REAL32 *ramp; /* used in εhift */ ) TRECTABLES; /* this structure holds all the memory pointers for data memory */ /* this includes intermediate results and work areas */ /* the memory areas need not be disjoint, two named areas may share memory: one name may be used by one part of recon, a second by another at a different time. typedef struct TRECMEMORY { UINT32 memtot; /* total memory used for data */ CHAR *chunkl; /* first memory chunk */ UINT32 sizel; I* size of first chunk */ CHAR *chunk2; I* second memory chunk */ UINT32 εize2; I* size of second chunk */ CHAR *chunk3; I* third memory chunk */ UINT32 εize3; /" size of third chunk */ CHAR *chunk4; I* fourth memory chunk */ UINT32 εize4; I* size of fourth chunk */ REAL32 •fansino; /* fan beam sinogram input data */ REAL32 *fansino2; /* fan beam sinogram input data */ REAL32 *rbtmem; /* rebinning temp memory */ REAL32 *viewl; /* v ew 1 size: cwidth */ REAL32 *view2,- / * view 2 size: cwidth */ REAL32 *view3; / * view 3 size: cwidth */ REAL32 *view4; / * view 4 size: cwidth */ REAL32 *gridtmp; /* temp area for gridding size cwidth */ REAL32 *cbviewl; /* cbviewl size: cwidth */ REAL32 *cbview2; /* cbview2 size: cwidth */ REAL32 *cbview3; /* cbview3 size: cwidth */ REAL32 *cbview4; /* cbview4 εize: cwidth */ REAL32 *shiftmem; εhift temp memory size: cwidth */ INT32 *vkx0; /* backp memory size: cwidth / 1* 1 INT32 *vky0; /* backp memory size: cwidth I 1* 1 REAL32 "wx; /* backp memory size: cwidth I 1* 1 REAL32 "wy; /* backp memory size: cwidth I 1* 1 REAL32 *vs; /' backp memory εize: cwidth / 1* 1 REAL32 *cbtempl; / used in fbackpcb size: cwidth*/ REAL32 *cbtemp2;/* used in fbackpcb εize: cwidth*/ REAL32 *cbcoords;/* used in cbcc size: cwidth * 8*/ REAL32 *xsino; /* intermediate rebinning sinogram */ REAL32 *xsino2; /* intermediate rebinning sinogram */ REAL32 *isino; /* intermediate rebinning sinogram */ REAL32 *isino2; /* intermediate rebinning sinogram */ REAL32 *psino; /* parallel beam sinogram */ REAL32 *psino2; /* parallel beam sinogram */ APPENDIX 1 REAL32 *fimage; /* Real image or Fourier transform of image */ INT16 *image; /* il6 output image */ } TREC_MEMORY; *********** * ***** ***** * end trec.h * *** *** ***** * ***** *** ** * * / APPENDIX 1 /* * File Name: trecMisc.c * * Author : Jon Harman * * Brief Description: Misc functions for tree. * * Copyright 1993 Imatron, Inc. * * Command Line Synopsis: * * Long Deεcription: * * Deficiencies / bugs: * * Return (status) codes, error messages: * * Abbreviations used: * * Revision History (latest updates first!): 3/15/93 (jonh) New. */ /* LINTLIBRARY *//* suppreεεes some unneeded lint messages */ /* 1.) "Imported" data types and defines: */ /* l.a.) Standard C include files */ ♦include <stdio.h> ♦include <math.h> ♦include <string.h> /* #include <sys/types.h> */ ♦ifdef MC860 ♦include <mcos.h> ♦include <sal_defs.h> ♦endif /* l.b.) Imatron ../include files */ ♦include " ../include/imatron.h" /* first Imatron include */ /* I.e.) Project include files */ ♦include "trec.h" /* l.d.) Other include files */ /* 2.) Externals defined in this file (declarations onry): */ FORWARD INT rfftshO; FORWARD INT rfft2dsh(); FORWARD INT allocmemO; /* 3.) "Imported" externals: */ /* 3.a.) Imported from standard C Library */ IMPORT CHAR *malloc() ; /* 3.b.) Imported from ../xxxxx */ /* 3.c.) Imported from other files in thiε dtrectory */ /* 3.d.) Imported from elsewhere */ /* 4.) "Private" data types, defines, data and code */ ♦ifdef MC860 IMPORT REAL32 εalcache[4]; ♦elεe ♦define SAL_NC 1 ♦define SAL_NCC 1 ♦define SAL_CCN 1 ♦define SAL_CNC 1 ♦define SAL_CN 1 ♦define SAL_CC 1 ♦define SAL_C 1 PRIVATE REAL32 εalcache[2048] ,- APPENDIX 1 ♦endif /* 5.) Exported Functions and Data: */ /* a εhell for rfft which includes inv and flip */ /* inv iε a boolean for inverse rather than the dir (+-1) used by Mercury */ /* * flip causes a 180deg εhift in the position of the spatial data by * multiplying the transform by +-1 */ /* doscale = TRUE does correct scaling */ INT rfftεh(f, n, inv, flip, doscale) REAL32 *f; INT n, inv, flip, doscale; { INT dir, i; REAL32 negl = -1, εcale, *ca = εalcache; if (inv) dir = -1; else dir = 1; if (flip tt inv) { vsmul(tf[2], 4, tnegl, tf[2], 4, n / 4) ; vsmul(tf[3], 4, tnegl, tf[3], 4, n / 4); } rfft(f, n, dir); if (flip && !inv) { vsmul(tf[2], 4, tnegl, tf[2], 4, n / 4) ; vsmul(tfΪ3], 4. tnegl, tf[3), 4, n / 4) ; } if (doscale) { if (inv) scale = 1.0 / (REAL) n; elεe scale = .5; vεmultf, 1, tscale, f, 1, n) ; ) return (0) ; ) /* thiε just does the flip from rfftsh */ EXPORT INT flip(f, n) REAL32 *f; INT n; { REAL32 negl = -1; vεmul(tf[2], 4, tnegl, tf[2], 4, n / 4) ; vεmul(tf[3], 4, tnegl, tf[3], 4, n / 4) ; return (0) ; } /* a εhell for 2D rfft which includes inv and flip */ INT rfft2dsh(f, nc, nr, inv, flip, doscale) REAL32 *f; INT nc, nr, inv, flip, doscale; { INT dir, i, j, itwo = 2, twonc = 2 * nc, ni, ii, jj, kk, mtwo=-2,n2; REAL32 negl = -1, εcale, two = 2.0,half = .5; APPENDIX 1 PRIVATE REAL32 cnq[4096] ; if(inv) dir = -1; else dir = 1; if (flip t inv) { for (i = 0; i < nr; i += 2) { /* even rows */ vsmuMtfd * nc + 2], 4, tnegl, tf[i * nc + 2], 4, nc / 4) ; vεmul(tfϊi * nc + 3], 4, tnegl, tfϊi * nc + 3] , 4, nc / 4); /* odd rows */ vsmul(tf[(i + 1) * nc + 4], 4, tnegl, tf[(i + 1) * nc + 4], 4, nc / 4 - 1); vεmul(tf[(i + 1) * nc + 5] , 4, tnegl, tf[(i + 1) * nc + 5] , 4, nc / 4 - 1); ) vεmul(tf[2 * nc] , 4 * nc, tnegl, tf[2 * nc] , 4 * nc, nr / 4) ; vsmul(tfΪ3 * nc], 4 * nc, tnegl, tfΪ3 * nc] , 4 * nc, nr / 4); vsmul(tfΪ2 * nc + 1], 4 * nc, tnegl, tf[2 * nc + 1] , 4 * nc, nr / 4); vεmul(tfΪ3 * nc + 1] , 4 * nc, tnegl, tfΪ3 * nc + 1] , 4 * nc, nr / 4); ) ♦if 0 if (flip t inv) { for (i = 0; i < nr; i += 2) { vsmuMtfd * nc + 2], 4, tnegl, tf[i * nc + 2], 4, nc / 4); vsmulitfϊi * nc + 3], 4, tnegl, tfϊi * nc + 3], 4, nc / 4) ; vsmul(tf[(i + 1) * nc] , 4, tnegl, tf[(i + 1) * nc + 4], 4, nc / 4); vsmul(tf[(i + 1) * nc + 1], 4, tnegl, tf[(i + 1) * nc + 5] , 4, nc / 4); > vsmul(tf[nr * nc + 2] , 4, tnegl, tf[nr * nc + 2], 4, nc / 4); vεmul(tfϊnr * nc + 3], 4, tnegl, tfϊnr * nc + 3], 4, nc / 4); } ♦endif ♦ifndef CSPI rfft2d(f,nc,nr,dir) ; ♦else if(dir == 1) { for(i=0;i<1024;i++) cnq[i] = -1.0; rft2fr_(f, cnq, titwo, f, tnr, tnc); /* do packing of cnq array into mercury format here */ ni = nr / 2 - 1; ii = -nc; jj = 2 * nc; vmov_(f + (nr - 1)* nc, tii, f + 2 * nc, tjj, tni); ii = nc; vmov_(f + nc + 1, tii, f + 3 * nc, tjj, tni); f[nc] = f[nc * nr / 2] ; ii = 1; vmov_(cnq, tii, f + 1, tnc, tnr); f[nc + 1] = cnq[nr]; ) elεe { /* do unpacking from mercury format col 1 to cnq array here */ /* something is fishy here, cnq is a nr * 2 complex array, yet I fill up only half of it. The output equals mercury though. */ ii = 1; vclr (cnq, 1 , nr * 2 ) ; vmov_(f + 1 , tnc, cnq, tii, tnr) ; APPENDIX 1 cnq[nr] = f[nc + 1] ; cnqϊnr + 1] = 0.0; cnqϊl] = 0.0; /* ni = nr / 2 - 1; vmov_(cnq+2, titwo, cnq+nr-2, tmtwo, tni) ; vmov_(cnq+3, titwo, cnq+nr-1, tmtwo, tni); thiε iε close, but not quite right. I give up! */ cnq[0] *= .5; n2 = nr * 2; vεmul_(cnq, tii, ttwo, cnq, tii, tn2); ni = nc / 2 - 1; /* fix up cols 0 and 1 */ ii = nc; jj = 2 * nc; vmov_(f + 3 * nc, tjj, f + nc + 1, tii, tni); jj = -nc; vneg_(f + nc + 1, tii, f + (nr - 1) * nc + 1, tjj, tni); ii = 2 * nc; jj = 1; vmov_(f + 2 * nc, tii, cnq + 2 * nr, tjj, tni); /* temp εtorage */ ii = 1; jj = -nc; vmov_(cnq + 2 * nr, tii, f + (nr - 1) * nc, tjj, tni); f[nc * nr / 2] = f[nc] ; ii = -nc; jj = nc; vmov_(f + (nr - 1) * nc, tii, f + nc, tjj, tni); f[l] = 0.0; f[nr * nc /2 + 1] = 0.0; rft2ir_(f, cnq, titwo, f, tnr, tnc) ; } ♦endif if (flip tt !inv) { for (i = 0; i < nr; i += 2) { vεmul(tf[i * nc + 2] , 4, tnegl, tf[i * nc + 2], 4, nc / 4); vsmuMtfd * nc + 3], 4, tnegl, tfϊi * nc + 3] , 4, nc / 4) ; vεmul(tf[(i + 1) * nc + 4] , 4, tnegl, tf[(i + 1) * nc + 4] , 4, nc / 4 - 1); vεmul(tf[(i + 1) * nc + 5] , 4, tnegl, tf[(i + 1) * nc + 5] , 4, nc / 4 - 1); } vεmul(tf[2 * nc] , 4 * nc, tnegl, tf[2 * nc] , 4 * nc, nr / 4); vεmul(tfΪ3 * nc] , 4 * nc, tnegl, tf[3 * nc] , 4 * nc, nr / 4); vεmul(tf[2 * nc + 1] , 4 * nc, tnegl, tf[2 * nc + 1] , 4 * nc, nr / 4); vεmul(tf[3 * nc + 1] , 4 * nc, tnegl, tf[3 * nc + 1] , 4 * nc, nr / 4); } if(doεcale) { if(inv) scale = 1.0 / ((REAL)nc * (REAL)nr) ; elεe εcale = .5; vsmul(f,l,tscale,f,l,nc * nr) ; } return(0) ; } PRIVATE INT imax(a, b) INT a, b; APPENDIX 1 if (a > b) return (a); return (b) ; allocate data memory. We calculate the sizes of the biggest chunks of memory needed. Then distribute the actual memory needs within the chunks. Note that there are usually two big chunks in use: fansino, xsino: first rebin εtep xsino, isino: second rebin step isino, pεino: final rebin εtep pεino, fimage: backprojection EXPORT INT allocmem(trecParams, trecMemory, dorebin) TREC_PARAMS *trecParams; TREC_MEMORY *trecMemory; INT dorebin; { INT i, fansize, psize, minviewsl, rsize, tεize, fεize; /* calc εizes needed for the chunks first */ if(dorebin) minviewsl = trecParams->minviews + 2 trecParams->nl; else minviewsl = 4; /* tsize iε the εize of temp memory chunk */ /* rebinning temp */ tsize = trecParams->rwidth; /* area for views and other data during backprojection, shared with rbtemp */ tsize = imax(tsize, trecParams->cwidth * 9); if(trecParams->cb) tsize = imax(tsize, trecParams->cwidth * (15 + NCALC)); tεize *= sizeof(REAL32) ; fansize = minviewsl * trecParams->nsamps * εizeof(REAL32) ,- psize = trecParams->rwidth * trecParams->pviews * εizeof(REAL32) ; rεize = imax(fansize, psize); /* εize for rebinning memory chunks*/ /* Fourier image size */ fsize = trecParams->fwidth * (trecParams->fwidth + 2) * sizeof(REAL32) ,- trecMemory->sizel = imax(fsize, rsize); trecMemory->size2 = rsize; trecMemory->εize3 = 4096;/* not used */ trecMemory->size4 = tsize; if(trecParamε->cb) { trecMemory->εize2 = rsize; trecMemory->size3 = rεize; trecMemory->εize4 = tεize; > /* for the 860 */ trecMemory->εizel ((4095 + trecMemory->εizel) / 4096) * 4096 trecMemory->εize2 ((4095 + trecMemory->εize2) / 4096) * 4096 trecMemory->εize3 ((4095 + trecMemory->size3) / 4096) * 4096 trecMemory->εize4 ((4095 + trecMemory->εize4) / 4096) * 4096 ♦ifdef MC860 trecMemory->chunkl = (CHAR *) memalign(4096, trecMemory->εizel) ; APPENDIX 1 i = mcntl(MC_CACHE, trecMemory->chunkl, trecMemory->sizel) ; if (i) printf("mcntl error for chunkl.\n"); trecMemory->chunk2 = (CHAR *) memalign(4096, trecMemory->size2) ; i = mcntl(MC_CACHE, trecMemory->chunk2, trecMemory->size2) ; if (i) printf("mcntl error for chunk2.\n"); trecMemory->chunk3 = (CHAR *) memalign(4096, trecMemory->size3) ; i = mcntl(MC_CACHE, trecMemory->chunk3, trecMemory->size3) ; if (i) printf("mcntl error for chunk3.\n") ; trecMemory->chunk4 = (CHAR *) memalign(4096, trecMemory->size4) ; i = mcntl(MC_CACHE, trecMemory->chunk4, trecMemory->εize4) ; if (i) printf("mcntl error for chunk4.\n") ; ♦else trecMemory->chunkl = (CHAR *) malloc(trecMemory->εizel) ; - trecMemory->chunk2 = (CHAR *) malloc(trecMemory->size2) ,- trecMemory->chunk3 = (CHAR *) malloc(trecMemory->size3) ; trecMemory->chunk4 = (CHAR *) malloc(trecMemory->size4) ; ♦endif if ( !trecMemory->chunkl) { printf("tree. Cannot get memory(%d) for chunkl, memtot:%d.\n", trecMemory->sizel, trecMemory->memtot) ,- return (-1); } trecMemory->memtot += trecMemory->sizel; if ( !trecMemory->chunk2) { printf("tree. Cannot get memory(%d) for chunk2, memtot:%d.\n", trecMemory->size2, trecMemory->memtot) ; return (-1) ; } trecMemory->memtot += trecMemory->size2; if ( !trecMemory->chunk3) { printf("tree. Cannot get memory(%d) for chunk3, memtot:%d.\n", trecMemory->εize3, trecMemory->memtot) ; return (-1) ; } trecMemory->memtot += trecMemory->size3; if (!trecMemory->chunk4) { printf("tree. Cannot get memory(%d) for chunk4, memtot:%d.\n", trecMemory->size4, trecMemory->memtot) ; return {-1) ; ) trecMemory->memtot += trecMemory->size ; * next we apportion out the data areas inside the chunk. Thiε iε not εo * easy. Any changes in program flow must carefully be examined for * effect on memory allocation trecMemory->fansino = (REAL32 *) trecMemory->chunkl; trecMemory->xsino = (REAL32 *) trecMemory->chunk2; trecMemory->isino = (REAL32 *) trecMemory->chunkl; trecMemory->psino = (REAL32 *) trecMemory->chunk2; trecMemory->rbtmem =(REAL32 *) trecMemory->chunk4; trecMemory->shiftmem = (REAL32 *) trecMemory->chunk ; trecMemory->vkxO = (INT32 *) (trecMemory->εhiftmem + trecParams->cwidth) ; trecMemory->vky0 = trecMemory->vkx0 + trecParams->cwidth/2; APPENDIX 1 trecMemory->wx = (REAL32 **) (trecMemory->vky0 + trecParams->cwidth/2) trecMemory-> y = trecMemory->wx + trecParams->cwidth/2; trecMemory->vε = (REAL32 *) trecMemory-> y + trecParams->cwidth / 2; trecMemory->viewl = (REAL32 *) trecMemory->vs + trecParams->cwidth / 2; trecMemory->view2 = trecMemory->viewl + trecParams->cwidth; trecMemory->view3 = trecMemory->view2 + trecParams->cwidth; trecMemory->view4 = trecMemory->view3 + trecParams-xrwidth; trecMemory->gridtπrp = trecMemory->view4 + trecParams->cwidth; trecMemory->fimage = (REAL32 *) trecMemory->chunkl; trecMemory->image = (INT16 *) trecMemory->chunkl,- if(trecParams->cb) { trecMemory->fansino = (REAL32 *) trecMemory->chunk2; trecMemory->fansino2 = (REAL32 ) trecMemory->chunk3; trecMemory->xsino = (REAL32 *) trecMemory->chunkl,- trecMemory->xsino2 = (REAL32 *) trecMemory->chunk2; trecMemory->isino = (REAL32 *) trecMemory->chunk3; trecMemory->isino2 = (REAL32 *) trecMemory->chunkl; trecMemory->psino = (REAL32 *) trecMemory->chunk2; trecMemory->psino2 = (REAL32 *) trecMemory->chunk3; trecMemory->cbviewl trecMemory->view4 trecParams->cwidth; trecMemory->cbview2 trecMemory->cbviewl + trecParams->cwidth; trecMemory->cbview3 trecMemory->cbview2 + trecParams->cwidth; trecMemory->cbview4 trecMemory->cbview3 + trecParams->cwidth; trecMemory->cbtempl trecMemory->cbview4 + trecParams->cwidth; trecMemory->cbtemp2 trecMemory->cbtempl + trecParams->cwidth; trecMemory->grid .t.mp. trecMemory->cbt-e_mp.2_ + trecParams-xrwidth; trecMemory->cbcoords = trecMemory->gridtmp + trecParams->cwidth; } return (0) /* * fill in extra views for a fan beam sinogram. Thiε version assumes that * sampoffεet = 0, hence that -iεigma = width - isigma - 1 * view: view number of view to fillin, * viewO: first existing view * ngood: number of existing views * width: width of views * fanang: fanangle in radians */ EXPORT INT fanfillin(sino, view, viewO, ngood, nviews, width, fanang) REAL32 *sino; INT view, viewO, ngood, nviews, width; REAL fanang; { INT i, j, k, n, isigma, iview, lview = viewO + ngood - 1; INT vhalf = viewO + ngood/2; REAL dO, dl, dsigma, sigma, sigmaO, beta, rview; REAL32 *εinol = εino + view * width; /* * we use the relation sino(εigma,beta) = εino(-εigma,PI + beta + 2 * * εigma) if εampoffεet = 0 then -εigma will fall at an integer we do * linear interpolation between views */ dεigma = fanang / (width - 1) ; εigmaO = -fanang / 2.0; beta = view * TWOPI / (REAL) nviews; for (isigma = 0, sigma = sigmaO; isigma < width; isigma++, sigma += dsigma) if (view > vhalf) rview = (beta - PI + 2 * sigma) * nviews / TWOPI; elεe APPENDIX 1 rview = (beta + PI + 2 * εigma) * nviews / TWOPI; iview = rview; if ((iview < viewO) || (iview >= lview)) sinol[iεigma] = 0.0; /* outside */ else { dO = rview - iview; dl = 1 - dO; k = iview * width + width - isigma - 1; sinol[isigma] = dl * sino[k] + dO * εino[width + k] ; } } return (0) ; } /* read in the input sinogram from a file. Can be fan beam or parallel. returns number of views actually read, or -1 if not enough */ EXPORT INT readinput(fansino, psino, trecParams, dorebin, skip, fp) REAL32 *fansino, *psino; TREC_PARAMS *trecParams; INT dorebin, skip; FILE *fp; { INT nsamps = trecParams->nsamps, nl = trecParams->nl; INT psize, ssize, viewsread, nclr; REAL32 *readstart; if (dorebin) { if (skip) fread(fansino, sizeof(REAL32) , εkip * nsamps, fp) ; vclr(fansino, 1, nl * nsamps); readstart = fansino + nl * nsamps; ssize = (trecParams->minviews + nl) * nsamps; nclr = ssize; ssize = fread(readstart, εizeof(REAL32) , εεize, fp) ; viewsread = ssize / nsamps; nclr = nclr - viewsread * nsamps; if(nclr > 0) vclr(fansino + (viewsread + nl) * nsamps, 1, nclr); if(viewsread < trecParams->minviews) viewsread = -1; } else { psize = trecParams->rwidth * trecParams->pviews; εεize = fread(psino, εizeof(REAL32) , psize, fp) ; viewsread = ssize / trecParams->rwidth; if(viewsread < trecParams->pviews) viewsread = -1; ) return(viewsread) ,- } /* mformat: put the inverse fft matrix into Mercury real 2D FFT format. See the Mercury documentation for a description of their format. One wrinkle is that I have εtored the last complex column as the last two rows. */ INT mformat(image, nx, ny) REAL32 *image; INT nx, ny; {INT i; REAL32 t; /* deal with the firεt complex column */ image l O] *= 2.0 ; APPENDIX 1 for(i = 1; i < ny/2;i++) { imaged * nx] += image[(ny - i) * nx] ; imageϊi * nx + 1] -= image[(ny - i) * nx + 1] ; } t = image[ny I I * nx] ; for(i=ny/2 - l;i > 0;i—) { image[i * 2 * nx] = imaged * nx] ; imageϊ (i * 2 + 1) * nx] = imaged * nx + 1] ; ) image[nx] = 2.0 * t; /* factor of 2 seems to improve things */ /* the last complex column is stored as two extra rows. it gets stuffed into the second column of the packed image */ for(i=l;i < ny/2; i++) { image[nx * ny + 2 * i] += image[nx * ny + (ny - i) * 2); imageϊnx * ny + 2 * i + 1] -= image[nx * ny + (ny - i) * 2 + 1] ; } ford = 1; i <ny/2;i++) { image[nx * 2 * i + 1] = image[nx * ny + 2 * i] ; imageϊnx * (2 * i + l) + l] = image[nx * ny + 2 * i + 1] ,- ) image[1] = 2.0 * image[nx * ny] ; imageϊnx + 1] = 0.0; return{0) ; /* εhifttranεv: shift viewε in a εinogra . The basis of this algorithm is that the parallel beam sinogram when transformed becomes a polar coordinate version of the 2D fft of the image. Thus to εhift the image the Fourier shift theorem can be applied to the εinogram. I do this by multiplying F(u,v) by exp(-2PI*i*sh*u) * exp(-2PI*i*εv*v) ) . In polar coords u = r cos(view), v = r sin(view) . I use the ramp to create r's for each point in the view then multiply by a εcalar -2PI*εh*coε(view) (for εh) . Then I uεe vcos and vsin to get the real and i ag parts of the exp. This needs two shifts, one horiz, one vert. This is a much slower version then shifttrans, but it iε eaεy to implement in a view by view recon algorithm. This verεion εhiftε 2 views (4 views for cone beam) at once. We use the fact that sin(PI - angle) = sin(angle) cos(PI - angle) = -cos(angle). Thus the same cos and sin tables can be used for two angles at once. εhifttranεv(trecTables, trecMemory, trecParams, angle, viewO, viewl, view2, cbviewl, cbview2) TREC_TABLES *trecTables; TREC_MEMORY *trecMemory; TREC_PARAMS *trecParams; REAL angle; INT viewO; REAL32 *viewl, *view2; REAL32 *cbviewl, *cbview2; { REAL 2 rtempi,rtemp2; INT i, width = trecParams->cwidth, fr = trecParams->fr; REAL εh, εv; APPENDIX 1 REAL32 *ramp = trecTables->ramp; REAL32 *tmem = trecMemory->shiftmem; εh = trecParams->x0 * width / 2; if(trecParams->doflip) εh = -sh; sv = -trecParams->y0 * width / 2; if(fabs(sh) > 0.0) { rtempl = (TWOPI * εh * -coε(angle) ) / width; vεmul(ramp, 1, trtempl, tmem, 1, fr * 2); vcoε(tmem, 2, tmem, 2, fr) ; vsin(tmem + 1, 2,tmem + 1, 2, fr) ; cvmul(viewl + 2, 2,tmem + 2, 2, viewl + 2, 2, fr - 1,1); if(trecParams->cb) cvmuMcbviewl + 2, 2,tmem + 2, 2, cbviewl + 2, 2, fr - 1,1); /* view 0 iε a εpecial case. then viewl is at 0, view2 is at PI / 2. εo cos(angle) = 1 for viewl, = 0 for view2. for view2 this εhift iε not needed since tmem is a complex vector of all (1,0) 'ε. */ if(view0 != 0) { /* view2 (cbview2) is at PI - angle, cos(PI - angle) = -cos(angle) so the vsin above needs to be negated for view2 */ vneg(tmem + 1, 2, tmem + 1, 2, fr) ; cvmul(view2 + 2, 2,tmem + 2, 2, view2 + 2, 2, fr - 1,1); if(trecParams->cb) cvmul(cbview2 + 2, 2,tmem + 2, 2, cbview2 + 2, 2, fr - 1,1); ) ) if(fabs(εv) > 0.0) { rtempl = (TWOPI * εv * -εin(angle)) / width; vεmul(ramp, 1, trtempl, tmem, 1, fr * 2); vcos(tmem, 2, t em, 2, fr) ; vsin(tmem + 1, 2,tmem + 1, 2, fr) ; cvmul(viewl + 2, 2,tmem + 2, 2, viewl + 2, 2, fr - 1,1); if(trecParams->cb) cvmuMcbviewl + 2, 2,tmem + 2, 2, cbviewl + 2, 2, fr - 1,1); if(view0 != 0) { /* here εin(PI - angle) = sin(angle) */ cvmul(view2 + 2, 2,tmem + 2, 2, view2 + 2, 2, fr - 1,1); if(trecParams->cb) cvmul(cbview2 + 2, 2,tmem + 2, 2, cbview2 + 2, 2, fr - 1,1); elεe /* view 0 is a special caεe. then viewl iε at 0, view2 is at PI / 2. εo sin(angle) = 0 for viewl, = 1 for view2. */ { rtempl = (-TWOPI * εv) / width; vεmul(ramp, 1, trtempl, tmem, 1, fr * 2); vcoε(tmem, 2, tmem, 2, fr) ; vεin(tmem + 1, 2,tmem + 1, 2, fr) ; cvmul(view2 + 2, 2, mem + 2, 2, view2 + 2, 2, fr - 1,1); if(trecParams->cb) cvmul(cbview2 + 2, 2,tmem + 2, 2, cbview2 + 2, 2, fr - 1,1); ) return(0) ; ) /* init the Fourier image, as of now this just means zeroing it out */ APPENDIX 1 INT init_img(image, width) REAL32 * image; INT width; { vclr(image, 1, width * (width + 2)); return(0) ; } /* norm_image:prepare the final image. This entails: 1. Normalization to eliminate doming of image due to convolution in the transform domain. We multiply with the coefficientε εtored in imgwin. The doming iε separable so we can use a 1-D array to normalize the 2D image. Note that a εcale factor iε hidden into the imgwin array. 2. Adding a constant to the image if desired. (Siemens addε 24.) 3. Clipping the image to ctmin(O) and ctmax(4095) . 4. Fix to a 16 bit unsigned integer. 5. Optionally zero out any area of the image outside the recon area. */ INT norm_image(trecTables, trecMemory, trecParams, εkipint) TRECTABLES *trecTables; TRECMEMORY *trecMemory; TRECPARAMS *trecParams; INT skipint; /* if true, skip conversion to an integer */ { REAL reconr; REAL32 *imgwin = trecTables->imgwin, *fimage = trecMemory->fimage; REAL32 clipO, clipl; INT i, j, iwidth = trecParams->iwidth, fwidth = trecParams->fwidth; /* first divide the image by the transform of the window function */ j = (fwidth - iwidth) / 2; /* do the horizontal normalization */ ford = j;i < j + iwidth;i++) vmul(imgwin + j, l,fimage + fwidth * i + j, 1, fimage + fwidth * i + j, 1, iwidth) ; /* do the vertical normalization and squeese down image to iwidth x iwidth */ ford = j;i < j + iwidth;i++) vεmul(fimage + fwidth * i + j, 1, imgwin + i, fimage + iwidth * (i - j), 1, iwidth) ; /* add a constant */ if(trecParams->ctconst != 0.0) vsadd(fimage, 1, ttrecParams->ctconst, fimage, 1, iwidth * iwidth); if(εkipint) return(0); /* skip the converεion to an integer */ /* clip to 0 .. 4095 */ vclip(fimage, 1, ttrecParams->ctmin, ttrecParams->ctmax, fimage, 1, iwidth * iwidth) ; /* fix to intl6 */ vfix(fimage, 1, trecMemory->image, 1, iwidth * iwidth); /* zero out area outside of recon circle */ /* if iwidth != fwidth / 2 then an adjustment iε needed */ reconr = trecParams->reconr * 2.0 * trecParams->iwidth / (REAL) trecParams->fwidth; if(trecParams->zout) zero_out(trecMemory->image, trecParams->iwidth, reconr, trecParams->x0, trecParams->y0) ; return(0) ; } APPENDIX 1 /* zero out part of image outside of recon circle. coords are x,y. recon circle is (x,y) :x**2 + y**2 <= 1.0. image is centered at (xoff,yoff) width nmat. the integer image coordinates are changed to (x,y) nmat = 2 * reconr in x,y coords. */ EXPORT INT zero_out(image, nmat, reconr, xoff, yoff) UINT16 *image; INT nmat; REAL reconr, xoff, yoff; { INT i, j, k, 1; REAL dx, xO, y, xbeg, ys; UINT16 *line; dx = 2.0 * reconr / nmat; xO = xoff - reconr; y = yoff - reconr; for(j=0; <nmat;j++) {line = image + j * nmat; ys =y * y; if(ys > 1.0) {ford = 0;i < nmat;i++) lined] =.0;) else { xbeg = sqrt(1.0 - ys) ; k = (-xbeg - xO) / dx; if(k > nmat) k = nmat; ford = 0; i < k; i++) lined] = 0; 1 = (xbeg - xO) / dx; if(1 < k) 1 = k; if(1 < 0) 1 = 0; ford = l;i < nmat; i++) lined] = 0; ) y += dx; ) return(0) ; } /********************* End Of trecMisc.c ********************** APPENDIX 1 /* * File Name: trecRebin.c * * Author : Jon Harman * * Brief Description: Does rebinning based on interpolation tables. * * Copyright 1993 Imatron, Inc. * Command Line Synopsis: * * Long Description: * * Deficiencies / bugs: * * Return (status) cpdeε, error messages: * * Abbreviations used: * * Revision Hiεtory (lateεt updates first!): 6/14/93 (jonh) New. */ /* LINTLIBRARY *//* suppresses some unneeded lint messages */ /* 1.) "Imported" data types and defines: */ /* l.a.) Standard C include files */ ♦include <stdio.h> ♦include <math.h> ♦include <εtring.h> ♦ifndef CSPI ♦include <εyε/types.h> ♦endif ♦ifdef MC860 ♦include <mcos.h> ♦include <εal_defs.h> ♦endif /* l.b.) Imatron ../include files */ ♦include "../include/imatron.h" /* first Imatron include */ ♦include "../include/scanner_config.h" /* scanner config */ /* I.e.) Project include files */ ♦include "trec.h" /* l.d.) Other include files */ /* 2.) Externals defined in this file (declarations only): */ FORWARD INT trecRebinO; PRIVATE REAL weights() ; FORWARD INT allocmemO; /* 3.) "Imported" externals: */ /* 3.a.) Imported from standard C Library */ IMPORT CHAR *malloc() ; IMPORT REAL atθf(); IMPORT FILE *pu_fope () ; /* 3.b.) Imported from ../xxxxx */ /* 3.c.) Imported from other files in this dtrectory */ /* 3.d.) Imported from elsewhere */ /* 4.) "Private" data types, defines, data and code */ ♦ifdef MC860 IMPORT REAL32 εalcache[4] ; ♦elεe ♦define SAL_NC 1 ♦define SAL_NCC 1 ♦define SAL_CNC 1 APPENDIX 1 ♦define SAL_CN 1 ♦define SAL_CC 1 ♦define SAL_CCN 1 PRIVATE REAL32 εalcache[2048] ; ♦endif PRIVATE INT teεt = 0, εaveinter = 0; /* 5.) Exported Functions and Data: */ /* * This iε the main rebinning program. Itε input iε a fan beam εinogram * plus the rebinning tables. Its output iε the parallel beam εinogram */ EXPORT INT trecRebin(trecParams, trecTables, trecMemory) TRECPARAMS *trecParams; TRECTABLES *trecTables; TRECMEMORY *trecMemory; £ REAL32 beta, εigma, dεigma, sigmaO; REAL32 accum; REAL32 *phil, *fsl, *psil, *psi0, *is0, *isl, *islim, *psl; REAL32 *fansino, *xsino, *psino, *isino, *tmem; REAL32 *fansino2, *xsino2, *psino2, *isino2; /* the following are handy abbreviations for elements in trecParams */ INT nbeta, ntheta, nsigma, ns, minviews; INT nl2, nk2; INT ibeta, isigma, is; INT i, k, 1; INT minviewsl; CHAR fname[80] ; FILE *fp; REAL32 coeff; /* memory requirements. fansino: minviewsl * nsamps xsino: minviews * nsamps isino: pviews * rwidth psino: pviews * rwidth tmem: max of minviewsl, rwidth f nsino != xsino xsino != iεino psino != isino tmem != any other memory fansino = trecMemory->fansino; xεino = trecMemory->xsino; iεino = trecMemory->isino; psino = trecMemory->psino; fansino2 = trecMemory->fansino2; xsino2 = trecMemory->xsino2; isino2 = trecMemory->isino2; psino2 = trecMemory->psino2; tmem = trecMemory->rbtmem; minviews = trecParams->minviews; minviewsl = minviews + 2 * trecParams->nl; nl2 = 2 * trecParams->nl; nk2 = 2 * trecParams->nk; nbeta = trecParams->pviews * 2; ntheta = nbeta / 2; nsigma = trecParams->nsamps; ns = trecParams->rwidth; APPENDIX 1 /* if reverse we flip the εinogram. Obviously thiε is not optimized, rather it's just something quick and dirty to allow us to have the capability. */ if (trecParams->reverse) for (ibeta = 0; ibeta < minviewsl; ibeta++) { iε = ibeta * nsigma; for (iεigma = 0; iεigma < nεigma / 2; iεigma++) { accum = fansino[is + iεigmaJ ; fansino[is + iεigma] = fanεino[iε + nεigma - iεigma - 1] ; fansinoϊis + nsigma - iεigma - 1] = accum; if(trecParams->cb) { accum = fansino2 [is + iεigma] ; fanεino2[iε + isigma) = fansino2[is + nsigma - isigma - 1] ; fansino2Ϊis + nεigma - iεigma - 1] = accum; } ) ) /* optionally do 2D clipping, need tmem of length nsigma This used to be done at the end of rebinning. But I think putting it at the beginning is better. */ clip2d(fansino, tmem, minviewsl, nsigma, trecParams->clip2d) ; if(trecParams->cb) clip2d(fansino2, tmem, minviewsl, nsigma, trecParams->clip2d) ; /* now do the initial rebinning: from (sigma, beta) to (theta, sigma) */ btot(fansino, xsino, trecTables->phi, minviews, nsigma, nl2); if(trecParams->cb) btot(fansino2, xεino2, trecTables->phi, minviews, nsigma, nl2); /* next fold the information in the corners into the area used for the final output parallel sinogram */ if (trecParams->dofold) { if( !trecParams->cb) foldinter(xsino, trecTables->nnbeta, trecParams); else foldintercb(xsino, xsino2, trecTables->nnbeta, trecParams); ) if (saveinter) return(0); /* Now do the final interpolation from (theta, εigma) to (ε, theta) This goes from xsino to isino. The rows and columns are exchanged again. */ εtos(xsino, isino, trecTables, minviews, ns, nk2, ntheta); if(trecParams->cb) εtoε(xsino2, isino2, trecTables, minviews, ns, nk2, ntheta); /* * finally go from isino to pεino. Thiε involves transposing the data * and rotating */ tandrdεino, psino, ns, ntheta, trecParams->rot, trecParams->rscale) ,- if(trecParams->cb) tandr(isino2, pεino2, nε, ntheta, trecParams->rot, trecParams->rscale) ,- return ( 0 ) ,- APPENDIX 1 INT clip2d(fansino, tmem, minviewsl, nsigma, rclip2d) REAL32 *fansino;/* input εinogram */ REAL32 *tmem; /* εome temp memory of width nsigma */ REAL rclip2d; /* clip factor, 0 means don't do anything */ INT minviewsl, nsigma; /* length and width of sinogram */ { REAL32 clip2d, mclip2d, half = .5; INT ibeta, is; REAL32 *ca = εalcache, *cal = εalcache + 1024; if(rclip2d <= 0.0) return(O) ; if(nεigma > 1024) return(-l); clip2d = rclip2d; mclip2d = -clip2d; for (ibeta = 0; ibeta < minviewsl; ibeta++) { is = ibeta * nsigma; tmem[0] = 2 * fansino[is]; tmemϊnsigma - 1] = 2 * fansino[is + nsigma - 1] ; vadd(fansino + is, 1, fansino + is + 2, 1, tmem + 1, 1, nsigma - 2); ♦if CSPI tkclip2d(fansino + is, tmem, tmclip2d, tclip2d, tnsigma) ; ♦elεe vsmulx(tmem, 1, thalf, ca, 1, nsigma, SAL_NC) ; vsubx(ca, 1, fansino + is, 1, cal, 1, nsigma, SAL_CNC) ; vclipx(cal, 1, tmclip2d, tclip2d, cal, 1, nsigma, SAL_CC) ; vaddx(ca, 1, cal, 1, fansino + is, 1, nsigma, SAL_CCN) ,- ♦endif ) return(0) ; ) /* btot creates the intermediate sinogram (beta to theta) . It starts with a nsamps x minviews + 2*nl fan beam εinogram. (sigma,beta) It results in a minviews x nsamps intermediate sinogram. (theta,sigma) Note that the εinogram has its rows and columns exchanged in this step. The 2*nl extra input rows are needed for the interpolation and disappear after this step. */ INT btot(fansino, xεino, phi, minviews, nsigma, nl2) REAL32 *xsino, *fansino, *phi; INT minviews, nsigma, nl2; { INT i, isigma, w; w = minviews + nl2; /* width of the tranεpoεed matrix */ /* firεt tranεpoεe the input matrix */ tranε(fansino, 1, xsino, 1, nsigma, w) ; /* convolve the rows with the phi function */ for(iεigma = 0;iεigma < nεigma;iεigma++) { myconv(xεino + iεigma * w, 1, phi + iεigma * nl2, 1, xεino + iεigma * minviews, 1, minviews, nl2); ) return(0) ,- ) /* * foldinter folds the corners of the intermediate εinogram into the part APPENDIX 1 * that gets used in the final reεult. For each εample iεigma the pointε that are not in the final result are 0 .. nnbeta[isigma] - 1 and nnbeta[iεigma] + ntheta .. minviews - 1 */ INT foldinter(xsino, nnbeta, trecParams) TRECPARAMS *trecParams; REAL32 *xsino; UINT16 *nnbeta; { INT i, j, k, n, cfεlim = 0, cfend, npviews = 1, cfblim = 0; INT minviews, ntheta, nsamps, nnb; REAL w, wl, w2, xl, x2, x, dsigma, dtheta; REAL32 *cornerl, *coroer2, *finall, *final2, zero = 0.0, half = .5; CHAR εtr[100] ; ntheta = trecParams->pviews; nsampε = trecParams->nsampε; minviewε = trecParamε->minviewε; dsigma = trecParams->fanang / (nsampε - 1) ; dtheta = PI / ntheta; npviews = trecParams->npviews; cfslim = trecParams->cfslim; cfblim = trecParams->cfblim; if(test) { while(1) { printf("Enter i: ") ;gets(εtr) ;i = atoi(str); if(i < 0) break; printf("nnbeta[i] :%d, enter j:", nnbetad] ) ;gets(str) ; j = atoi(str) w = weightsd, j - nnbetad], ntheta, nsamps, trecParams->fanang) ,- k = nsampε - i - 1;/* thiε iε -εigma */ wl = weights(k, minviews - j - nnbetafk], ntheta, nsamps, trecParams->fanang) ; cornerl = xsino + i * minviews; corner2 = xsino + k * minviews + minviews; finall = xεino + k * minviews + nnbeta[k] - nnbetad) + ntheta; final2 = cornerl - nnbeta[k] + nnbeta[i] + minviews - ntheta; printf("w:%g cl:%g fl:%g c2:%g f2:%g\n", w, cornerl[j], finall[j], corner2[-j], final2[-j] ) ; ) printf("Enter npviews[%d] : ",npviews) ; gets(str) ,- if(εtrlen(str) ) npviewε = atoi(εtr); printf("Enter cfεlim[%d] :",cfslim) ; gets(str) ; if(εtrlen(εtr) ) cfslim = atoi(str); printf("Enter cfblim[%d] :".cfblim) ; getε(εtr) ; if(εtrlen(εtr) ) cfblim = atoi(str) ; } if(trecParamε->docf == 3) /* for cone beam zero out the cornerε */ { for (i = 0; i < nεamps; i++) { nnb = nnbeta[i] ; if(nnb > 0) vfilMtzero, xsino + i * minviews, 1, nnb); n = minviews - nnb - ntheta; if(n > 0) vfilMtzero, xsino + i * minviews + nnb + ntheta, 1, n) ; } } APPENDIX 1 if(trecParams->docf == 4) /* for cone beam zero out the center */ { for (i = 0; i < nsamps; i++) vfilMtzero, xsino + i * minviews + nnbeta[i], 1, ntheta); ) xl = trecParams->fanang; /* xl = fanang - is * dsigma */ for (i = 0; i < nεampε; i++) { k = nεamps - i - 1;/* this iε -εigma */ nnb = nnbetad]; /* at εample i first corner startε at 1, goeε to nnbetad) - 1 the firεt point (j=0) has a weight of 0 so can be ignored */ cornerl = xsino + i * minviews; /* at εample k εecond corner starts at inviewε - 1 goes to minviews - nnbeta[i] + 1, then last point is done separately, it always has a weight of .5 */ corner2 = xsino + k * minviews + minviews; finall = xεino + k * minviews + nnbeta[k] - nnb + ntheta; final2 = cornerl - nnbeta[k] + nnb + minviews - ntheta; if (i >= cfslim) cfend = 1; else cfend = (cfblim * (cfεlim - i)) / cfslim; if (cfend < npviews) cfend = npviews; /* j must start at 1 for corner2 and final2 addresses to be ok */ /* therefore always have npviews at least equal to 1 */ /* all those points up to cfend are deemed to be corner filled, hence do not need to be folded */ x2 = (cfend - nnb) * dtheta; for (j = cfend; j < nnb; j++) { /* w = weights (i , j - nnb, ntheta, nseaπps , trecParams->fanang) ,- */ x = (x2 + xl) / (2.0 * xl); if(x > 0.0) { w = x * x * (3.0 - 2.0 * x); if (w > 0.0) { finall[j] += w * (cornerl[j] - finall[j]) ; final2[- ] += w * (corner2 - ] - final2[-j] ) ,- final2[-nnb)) ; /* w is always .5 */ ) /* cone beam version of foldinter. has two sinograms to fold, corner area of one getε mapped to other */ INT foldintercb(xεino, xεino2, nnbeta, trecParams) TRECPARAMS *trecParams; REAL32 *xsino, *xεino2 ; UINT16 *nnbeta; { APPENDIX 1 INT i, j, k, n, cfslim = 0, cfend, npviews = 1, cfblim = 0; INT minviews, ntheta, nsamps, nnb; REAL w, wl, w2, xl, x2, x, dsigma, dtheta; REAL32 *cornerl, *corner2, *finall, *final2, *cor21, *cor22, *fin21, *fin22; REAL32 zero = 0.0, half = .5; CHAR str[100] ; ntheta = trecParams->pviews; nsamps = trecParams->nεampε; minviews = trecParams->minviewε; dεigma = trecParamε->fanang / (nsamps - 1) ; dtheta = PI / ntheta; npviews = trecParamε->npviews; cfεlim = trecParams->cfεlim; cfblim = trecParams->cfblim; xl = trecParams->fanang; /* xl = f nang - iε * dsigma */ for (i = 0; i < nsamps; i++) { k = nsamps - i - 1;/* this iε -εigma */ nnb = nnbetad]; /* at εample i first corner startε at 1, goeε to nnbetad] - 1 the firεt point (j=0) has a weight of 0 so can be ignored */ cornerl = xεino + i * minviews; cor21 = xsino2 + i * minviews; /* at sample k second corner starts at minviews - 1 goes to minviews - nnbetad] + 1, then last point is done separately, it always has a weight of .5 */ corner2 = xsino + k * minviews + minviews; cor22 = xsino2 + k * minviews + minviews; finall = xsino + k * minviews + nnbeta[k] - nnb + ntheta; final2 = cornerl - nnbeta[k] + nnb + minviews - ntheta; fin21 = xεino2 + k * minviewε + nnbeta[k] - nnb + ntheta; fin22 = cor21 - nnbeta[k] + nnb + minviews - ntheta; if (i >= cfslim) cfend = 1; else cfend = (cfblim * (cfslim - i)) / cfslim; if (cfend < npviews) cfend = npviews; /* j must start at 1 for corner2 and final2 addresses to be ok */ /* therefore always have npviews at least equal to 1 */ /* all those pointε up to cfend are deemed to be corner filled, hence do not need to be folded */ x2 = (cfend - nnb) * dtheta; for (j = cfend; j < nnb; j++) { x = (x2 + xl) / (2.0 * xl); if(x > 0.0) { w = x * x * (3.0 - 2.0 * x); if (w > 0.0) { finall[j] += w * (cor21[j] - finall[j]); final2[-j] += w * (cor22[-j] - final2[-j]); fin21[j] += w * (cornerlϊj] - fin21[j]); fin22[-j] += w * (corner2[-j] - fin22[-j]) ; ) ) x2 += dtheta; ) final2[-nnb] += .5 * (cor22[-nnb] - final2[-nnb] ) ,- /* w iε always .5 */ fin22[-nnb] += .5 * (corner2[-nnb] - fin22 ϊ-nnb] ) ,- /* w iε alwayε .5 */ xl -= dεigma; } APPENDIX 1 ) /* stos: εigma to ε interpolation. This takes an input sinogram (xsino) that has width minviews and produces an output sinogram of width ntheta and length ns, which is εtill transposed wrt the final output */ ♦ifndef CSPI INT εtoε(xsino, isino, trecTables, minviews, ns, nk2, ntheta) REAL32 *xsino; /* input εinogram, width iε minviewε */ REAL32 *iεino; /* output εinogram, width iε ntheta, length iε nε */ TRECTABLES *trecTableε; INT minviewε, nε, nk2, ntheta; { INT iε, iεigma, k; ' REAL32 *cachel = εalcache, coeff; for (iε = 0; iε < ns; is++) { iεigma = trecTables->nnsigma[iε] ; coeff = trecTables->psi[is] ; vsmulx(xεino + iεigma * minviews + trecTableε->nnbeta[iεigma] , 1, tcoeff, cachel, 1, ntheta, SAL_NC) ; for (k = 1; k < nk2; k++) { coeff = trecTables->psi[k * ns + is]; vsmax(xεino + (iεigma + k) * minviewε + trecTables->nnbeta[isigma + k] , 1, tcoeff, cachel, 1, cachel, 1, ntheta, SAL_NCC) ; ) ♦ifndef CSPI vmovx(cachel, 1, isino + iε * ntheta, 1, ntheta, SAL_CN) ; ♦elεe vmovx(cachel, 1, iεino + iε, ns, ntheta, SAL_CN) ; ♦endif } return (0) ; ) ♦else ♦define VSUMN 6 εtoε(xsino, iεino, trecTables, minviews, ns, nk2, ntheta) REAL32 *xsino; /* input εinogram, width is minviews */ REAL32 *iεino; /* output sinogram, width iε ntheta, length iε nε */ TRECTABLES *trecTables; INT minviews, ns, nk2, ntheta; { INT is, isigma, k, kl; REAL32 *tmem = εalcache, coeff; REAL32 *a0, *al, *a2, *a3, *a4, *a5, *b0, *bl, *b2, *b3, *b4, *b5; for (is = 0; iε < nε; iε++) { iεigma = trecTableε->nnεigma[iε] ; vclr(tmem, 1, ntheta); for(k = 0; k <= nk2 - VSUMN; k+=VSUMN) {aO = xεino + (iεigma + k) * minviews + trecTables->nnbeta[iεigma + k] ; al = xεino + (iεigma + k + 1) * minviewε + trecTableε->nnbeta[iεigma + k + 1] ,- a2 = xεino + (iεigma + k + 2) * minviewε + trecTableε->nnbeta[iεigma + k + 2]; a3 = xsino + (isigma + k + 3) * minviews + trecTableε->nnbeta[iεigma + k + 3]; a4 = xεino + (iεigma + k + 4) * minviews + trecTables->nnbeta[iεigma + k + 4] ; a5 = xsino + (isigma + k + 5) * minviews + trecTables->nnbeta[iεigma + k + 5] ; APPENDIX 1 bO = ttrecTables->pεi[k * nε + iε] ; bl = ttrecTableε->psi ϊ (k + 1) * ns + is] ,- b2 = ttrecTables->psiϊ (k + 2) * nε + iε] ; b3 = ttrecTableε->pεiϊ (k + 3) * nε + iε] ; b4 = ttrecTables->psiϊ (k + 4) * nε + iε] ; b5 = ttrecTableε->psiϊ (k + 5) * ns + is]; ♦if VSUMN == 3 tkvsum3(a0, al, a2, bO, bl, b2, tmem, tntheta) ; ♦elεe tkvεum6(a0, al, a2, a3, a4, a5, bO, bl, b2, b3, b4, b5, tmem, tntheta); ♦endif if(k + VSUMN * 2 > nk2) /* finiεh off any iεc remaining */ for(kl = k + VSUMN; kl < nk2; kl++) { coeff = trecTableε->pεi[kl * nε + iε] ; vεma(xεino + dεigma + kl) * minviewε + trecTableε->nnbeta[iεigma + kl] , 1, tcoeff, tmem, 1, tmem, 1, ntheta); ) ) vmov(tmem, 1, iεino + iε, ns, ntheta); ) return (0) ; ) ♦ifdef UNIX INT tkvsum3(a0, al, a2, bO, bl, b2, tmem, n) REAL32 *a0, *al, *a2, *b0, *bl, *b2; REAL32 *tmem; INT *n; { vεma(a0, 1, bO, tmem, 1, tmem, 1, *n) ; vsma(al, 1, bl, tmem, 1, tmem, 1, *n) ; vεma(a2, 1, b2, tmem, 1, tmem, 1, *n) ; } ♦endif ♦endif ♦if 0 INT stos(xsino, isino, trecTables, minviews, ns, nk2, ntheta) REAL32 *xsino; /* input sinogram, width is minviews */ REAL32 *isino; /* output εinogram, width is ntheta, length iε nε */ TRECTABLES *trecTableε; INT minviews, ns, nk2, ntheta; { INT is, isigma, k; REAL32 cache[2056], coeff; REAL32 rzero = 0.0,rone = 1.0; INT32 il=l,flip = 0; INT32 d, nl; INT32 bufl=l, buf2=2, nbuf=2; ♦define BUFFERSIZE (700) for (d = 0; d < ntheta; d += BUFFERSIZE) { nl = ntheta - d; if(nl > BUFFERSIZE) nl = BUFFERSIZE; for (is = 0; is < nε; is++) { iεigma = trecTables->nnsigma[iε] ; coeff = trecTableε->pεi[iε] ; vεmεa_εc_ (xεino + isigma * minviews + trecTables->nnbeta[isigma] + d. APPENDIX 1 til, tcoeff, trzero, tbufl, tni, tnbuf, cache); for (k = 1; k < nk2; k++) { coeff = trecTables->psi[k * nε + iε]; vεmεa_εc_ (xεino + (iεigma + k) * minviewε + trecTableε->nnbeta[iεigma + k] + d, til, tcoeff, trzero, tbuf2, tni, tnbuf, cache); vadd_ccc_ (tbufl, tbuf2, tbufl, tni, tnbuf, cache); flip = (flip + 1) t 1; if(flip) vεm2εa_εcc_ (xεino + (isigma + k) * minviewε + trecTableε->nnbeta[iεigma + k] + d, til, tcoeff, tbufl, trone, trzero, tbuf2, tni, tnbuf, cache) ; elεe vεm2εa_εcc_ (xεino + (iεigma + k) * minviewε + trecTables->nnbeta[iεigma + k]+d, til, tcoeff, tbuf2, trone, trzero, tbufl, tni, tnbuf, cache) ; */ /* if(flip) vmov_cs_ (tbuf2, iεino + iε + d * ns, tns, tni, tnbuf, cache); else vmov_cs_ (tbufl, isino + iε + d * ns, tns, tni, tnbuf, cache); vmov_cs_ (tbufl, isino + is + d * ns, tns, tni, tnbuf, cache); ) ) return (0) ; } ♦endif /* tandr transpose and rotate the output εinogram. for CSPI the tranεpose does not εpeed things up so we eliminate it. A compilcation is that the εinogram iε a 180 degree parallel εino. So a view at theta + 180 equals reverεe of view at theta. */ INT tandrdεino, pεino, ns, ntheta, rot, rscale) REAL32 *iεino, *pεino;/* input, output */ INT nε, ntheta, rot; REAL rscale; { INT rotl, itheta, k; REAL32 scale; εcale = rεcale; /* rot can be larger than ntheta : ntheta repreεents a rotation of 180 deg */ rotl = rot % ntheta; /* firεt tranεpoεe the viewε. It'ε faεteεt to do thiε uεing Mercury's routine */ ♦ifndef CSPI mtrans(iεino, 1, pεino, 1, ntheta, nε) ; vmov(pεino, 1, iεino, 1, ntheta * ns) ; ♦endif for (itheta = 0; itheta < ntheta; itheta++) /* itheta iε the εource view */ { k = itheta - rotl; /* k iε the destination view */ if (k < 0) k += ntheta; /* see if the pointε in the view need to be reverεed */ if (((itheta < rot) tt (rot < ntheta)) || ((itheta >= rot - ntheta) tt (rot >= ntheta) ) ) APPENDIX 1 {/* yes, reverse the view */ if (scale == 1.0) vmovdsino + itheta * ns + (ns - 1), -1, psino + k * ns + l, 1, nε - 1); elεe vεmul(iεino + itheta * ns + (nε - 1), -1, tscale, psino + k * nε + l, 1, nε - 1); pεino[k * nε] = 0.0; } elεe {/* no, εtraight copy */ if (εcale == 1.0) vmov(iεino + itheta * nε, 1, psino + k * ns, 1, ns) ; else vεmul(iεino + itheta * ns, 1, tscale, psino + k * ns, 1, ns) ; ) } return(0) ; ) /* calculate the weights for point in intermediate εinogram */ PRIVATE REAL weightεdε, it, ntheta, nεigma, f nang) INT is, it, ntheta, nsigma; REAL f nang; { PRIVATE INT init = 1; PRIVATE REAL32 sigmaO, dsigma, dtheta, constl, maxbeta, bO, fana; REAL32 εigma, beta, x, εigma2, w; if (init) { εigmaO = -fanang / 2.0; dsigma = f nang / (nsigma - 1); dtheta = PI / ntheta; conεtl = PI / 2.0 - fanang / 2.0; maxbeta = PI / 2.0 + fanang / 2.0; bO = PI / 2.0; fana = f nang; init = 0; ) εigma = is * dsigma + εigmaO; beta = it * dtheta - εigma - bO; if(teεt) printf("beta:%g εigma:%g\n", beta, εigma); if (beta < 0.0) { beta = -beta; εigma = —εigma; ) x = maxbeta - beta; if (x <= 0.0) return (0.0); εigma2 = 2.0 * εigma; if(test) printf("beta:%g constl-εigma2:%g\n", beta, constl- εigma2) ; if (beta <= conεtl - sigma2) return (1.0); x = x / (fana + εigma2) ; w = x * x * (3.0 - 2.0 * x); if(teεt) printf("x:%g w:%g\n", x, w) ; /* (fana + it * dtheta - is * dsigma) / (2.0 * (fana - is * dsigma))),- */ return(w) ; ) /* an add hoc routine to clean out εome garbage in corner fill area */ APPENDIX 1 EXPORT INT clean_dead(sino, nl, nviews, nsampε, docf) REAL32 *εino; INT nl, nviews, nsampε, docf; { INT v, ε, vO; if(docf == 1) /* 100ms */ { vO = 167 + nl; for{s=0;ε<48;ε+=6,v0-=2) for(v=v0;v>v0-15;v—) vclr(εino+v * nεampε + ε, 1, 6); vO = 734 + nl; for(ε=816;ε<nεamps;ε+=6,v0-= ) for(v=v0;v>v0+15;v++) vclr(sino+v * nεamps + ε, 1, 6); ) return(0) ; ) ♦ifndef CSPI /* I have had problems with mercury's convolution routine. Here is my own. It seems to go faster than mercury's. The speedup provided by the esal routines (verses sal in myconv)is .25 sec (1.10 vs 1.35) . */ myconv(a,i,b,j,c,k,n,p) REAL32 *a, *b, *c; INT32 i, j, k, n, p; { INT u,v; vεmulx(a,i,b,εalcache,1,n,SAL_NC) ,- for(v=l;v<p;v++) vεmax(a + v, i, b + v * j, εalcache, 1, εalcache, 1, n,SAL_NCC); vmovx(εalcache, 1, c, k, n,SAL_CN); ) ♦elεe myconv(a,i,b,j,c,k,n,p) REAL32 *a, *b, *c; INT32 i, j, k, n, p; { INT u,v; REAL accum; REAL32 zero = 0.0, one = 1.0; INT32 bufl = 1; INT32 buf2 = 2; INT32 nbuf = 2; STATIC REAL32 cache[2056]; INT32 nl, d, flip = 0; if((i == 1) tt (p == 6)) {tkconv6(a, b, b + 1, b + 2, b + 3, b + 4, b + 5, c, tk, tn) ; return(0) ; ) ♦define BUFFERSIZE (700) for (d=0; d < n; d+=BUFFERSIZE) { nl = n - d; if(nl > BUFFERSIZE) nl = BUFFERSIZE; APPENDIX 1 vεmsa_sc_ (a + (d * i) , ti, b, tzero, tbuf2, tni, tnbuf, cache); for (v = 1; v < p;v++) { vεmεa_εc_ (a + v + (d * i) , ti, b + v * j, tzero, tbufl, tni, tnbuf, cache); vadd_ccc_ (tbufl, tbuf2, tbuf2, tni, tnbuf, cache); flip = (flip + 1) t 1; if(flip) vsm2εa_εcc_ (a + v + (d * i) , ti, b + v * j, tbuf2, tone, tzero, tbufl, tni, tnbuf, cache) ; elεe vεm2εa_εcc_ (a + v + (d * i) , ti, b + v * j, tbufl, tone, tzero, tbuf2, tni, tnbuf, cache); */ } I* if(flip) vmov_cε_ (tbufl, c + (d * k) , tk, tni, tnbuf, cache); else vmov_cs_ (tbuf2, c + (d * k) , tk, tni, tnbuf, cache); */ vmov_cs_ (tbuf2, c + (d * k) , tk, tni, tnbuf, cache); ) } ♦endif ♦if 0 ♦define TSIZE 16384 ♦define WINC 32 /* this is not quite as fast as mtrans */ ymtrans(a,i,c,k,m,n) REAL32 *a, *c; INT32 i, k, m, n; { INT w, wi, rinc, r, ri, t; PRIVATE REAL32 temp[TSIZE] ; if((i != 1) || (k != 1)) { for(w = 0; w < m; w++) vmov(a + i * w, i * m, c + k * n * w, k, n) ; return; ) for(w = 0; w < m; w += WINC) { wi = m - w; if(wi > WINC) wi = WINC; if(wi == 1) vmov(a + w, , c + n * w, 1, n); elεe { rinc = TSIZE / wi; if(rinc > n) rinc = n; for(r = 0;r < n;r += rinc) { ri = n - r; if(ri > rinc) ri = rinc; for(t = 0;t < rinc; t++) vmov(a + (r + t) * m + w, 1, temp + t * wi, 1, wi); for(t = 0;t < wi;t++) vmov(temp + t, wi , c + (w + t) * n + r, 1 , ri) ; ) } APPENDIX 1 ) ) ♦endif /********************* End Of trecRebin. c **********************/ APPENDIX 1

Claims: HAT IS CLAIMED IS 1. A method for correcting cone beam error in an image reconstructed from data in a sinogram acquired from a fan beam computer tomography X-ray system, the method comprising the following steps: (a) rebinning fan beam data acquired from said system into parallel beam format, said step of rebinning including the steps of : (1) executing a first one-dimensional interpolation of columns in said fan beam data sinogram to generate an intermediate sinogram having a rectangular portion that includes non-redundant X-ray data and having first and second corner portions that include redundant X-ray data; (2) weighting said redundant data in said intermediate sinogram such that a sum of a redundant X-ray weight plus a central X-ray weight is unity, wherein said redundant data are folded over into said rectangular portion such that said weighted central X- ray plus said weighted redundant X-ray replaces said central X-ray value in said intermediate sinogram; (3) executing a second one-dimensional interpolation of rows in said intermediate sinogram, wherein said fan beam data are now represented in a parallel beam sinogram that includes said redundant data folded into said rectangular portion; and (b) reconstructing data acquired by said fan beam CT system, said step of reconstructing including the steps of: (1) filtering with a parallel beam kernel said parallel beam sinogram data for each view therein; (2) circularly shifting data resulting from said step Kb) (1) ,- (3) transforming data resulting from said step Kb) (2) ; (4) replicating data resulting from said step Kb) (3) ; (5) multiplying by an interpolation filter data resulting from said step 1(b) (4) ; (6) using a gridding function, gridding data resulting from said step 1(b) (5) into a Fourier image at an angle corresponding to the view angle; (7) convolving each view in said step 1(b) (6) with the transform of a cone beam weight function by multiplying by each non-zero coefficient of the weight function and gridding at an offset from the view angle into a Fourier image; (8) repeating steps (b) (1) through (b) (7) for each said view; (9) forming a preliminary image by taking a two- dimensional inverse Fourier transform of said views; (10) extracting a center portion of said preliminary image; (11) forming a reconstructed image by multiplying said preliminary image with its center portion extracted by an inverse of the transform of said gridding function; wherein said reconstructed image is substantially free of cone beam error. 2. The method of claim 1, wherein at step 1(a) (2) , said step of weighting is accomplished using short scan fan beam reconstruction weights. 3. For use with a parallel beam algorithm that corrects cone beam error in an image reconstructed from data in a sinogram acquired from a fan beam computer tomography X-ray system, a method for rebinning said data in said sinogram into parallel beam format, the method comprising the following steps : (a) executing a first one-dimensional interpolation of columns of the fan beam data sinogram to generate an intermediate sinogram having a rectangular portion that includes non-redundant data, and having first and second corner portions that include redundant data; (b) weighting said redundant data in said intermediate sinogram such that a sum of a redundant X-ray weight plus a central X-ray weight is unity, wherein said redundant data are folded over into said rectangular portion such that said weighted central X-ray plus said weighted redundant X-ray replaces said central X- ray value in said intermediate sinogram; and (c) executing a second one-dimensional interpolation of rows in said intermediate sinogram, wherein said fan beam data are now represented in a parallel beam sinogram that includes said redundant data folded into said rectangular portion. 4. The method of claim 3, wherein at step 3(b) , said step of weighting is accomplished using short scan fan beam reconstruction weights. 5. A method for reducing cone beam error in reconstructing an image from data acquired from a fan beam computer tomography X-ray system and rebinned into parallel beam sinogram, the method including the following steps: (a) filtering with a parallel beam kernel said parallel beam sinogram data for each view therein; (b) circularly shifting data resulting from said step 5(a) ; (c) transforming data resulting from said step 5(b) ; (d) replicating data resulting from said step 5(c) ; ; -i2o- (e) multiplying by an interpolation filter data resulting from said step 5 (d) ; (f) using a gridding function, gridding data resulting from said step 5(e) into a Fourier image at an angle corresponding to the view angle; (g) convolving each view in step 5(f) with the transform of a cone beam weight function by multiplying by each non-zero coefficient of the weight function and gridding at an offset from the view angle into a Fourier image; (h) repeating said steps (a) through (g) for each view; (i) forming a preliminary image by taking a two- dimensional inverse Fourier transform of said views; (j) extracting a center portion of said preliminary image; (k) forming a reconstructed image by multiplying said preliminary image with its center portion extracted by an inverse of the transform of said gridding function; wherein said reconstructed image is substantially free of cone beam error. 6. An apparatus for correcting cone beam error in an image reconstructed from data in a sinogram acquired from a fan beam computer tomography X-ray system, the apparatus comprising: (a) means for rebinning fan beam data acquired from said system into parallel beam format, said means for rebinning including: (1) means for executing a first one-dimensional interpolation of columns of the fan beam data sinogram to generate an intermediate sinogram having a rectangular portion that includes non-redundant data, and having first and second corner portions that include redundant data; (2) means for weighting said redundant data such that a sum of a redundant ray weight plus a central ray weight is unity, wherein said redundant data are folded over into said rectangular portion of said intermediate sinogram such that a sum of said weighted central ray plus said weighted redundant ray replaces said central ray value in said intermediate sinogram; (3) means for executing a second one-dimensional interpolation of rows in said intermediate sinogram, wherein said fan beam data are now represented in a parallel beam sinogram that includes said redundant data folded into said rectangular portion; and (b) means for reconstructing views acquired by said fan beam CT system, said means for reconstructing including: (1) means for filtering with a parallel beam kernel said parallel beam sinogram for each view therein; (2) means for circularly shifting output data from said means for filtering; (3) means for transforming output data from said means for circularly shifting; (4) means for replicating output data from said means for transforming; (5) means for multiplying by an interpolation filter output data from said means for replicating; (6) gridding function means for gridding output data from said means for multiplying into a Fourier image at an angle corresponding to the view angle; (7) means for convolving each view in output data provided by said gridding function means with the transform of a cone beam weight function by multiplying by each non-zero coefficient of the weight function and gridding at an offset from the view angle into a Fourier image; (8) means for subjecting each such view to said means described in (b) (1) through (b) (4) ; (9) means for forming a preliminary image by taking a two-dimensional inverse Fourier transform of said views; (10) means for extracting a center portion of said preliminary image; (11) means for forming a reconstructed image by multiplying said preliminary image with its center portion extracted by an inverse of the transform of said gridding function; wherein said reconstructed image is substantially free ne beam error.

Inventors: HARMAN JONATHAN W, HARMAN, JONATHAN, W.
Applicants: IMATRON INC, IMATRON, INC.
Application year: 1994
Main classification: G06F15
IPC codes: A61B6, G01N23, G06Q50, G06T1, G06T11